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We compute the production rate both at a semi-classical level, viewing Schwinger pair production... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_77632669" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We analyze the pair production of charged particles in two-dimensional Anti-de Sitter space (AdS_2) with a constant, uniform electric field. We compute the production rate both at a semi-classical level, viewing Schwinger pair production as a tunneling event, and at the full quantum level, by extracting the imaginary part of the one-loop amplitude. In contrast to the usual Schwinger pair production in flat space, pair production in AdS_2 requires a sufficiently large electric field E^2&gt; M^2+1/4 in order to overcome the confining effect of the AdS geometry -- put in another way, the presence of an electric field E raises the Breitenlohner-Freedman bound to M^2 &gt; -1/4 + E^2. For E greater than this threshold, the vacuum is unstable to production of charged pairs in the bulk. We expect our results to be helpful in constructing supersymmetric AdS_2 X S^2 perturbative string vacua, which enter in the near-horizon limit of extremal charged black holes. Although the generalized Breit...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/77632669" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="226918ac75a18b3cd2471a6b3d43d113" rel="nofollow" data-download="{"attachment_id":84949761,"asset_id":77632669,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/84949761/download_file?st=MTczMjQyMzQ5Nyw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="37740253" href="https://ens.academia.edu/JanTroost">Jan Troost</a><script data-card-contents-for-user="37740253" type="text/json">{"id":37740253,"first_name":"Jan","last_name":"Troost","domain_name":"ens","page_name":"JanTroost","display_name":"Jan Troost","profile_url":"https://ens.academia.edu/JanTroost?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_77632669 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="77632669"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 77632669, container: ".js-paper-rank-work_77632669", }); 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We compute the production rate both at a semi-classical level, viewing Schwinger pair production as a tunneling event, and at the full quantum level, by extracting the imaginary part of the one-loop amplitude. In contrast to the usual Schwinger pair production in flat space, pair production in AdS_2 requires a sufficiently large electric field E^2\u0026gt; M^2+1/4 in order to overcome the confining effect of the AdS geometry -- put in another way, the presence of an electric field E raises the Breitenlohner-Freedman bound to M^2 \u0026gt; -1/4 + E^2. For E greater than this threshold, the vacuum is unstable to production of charged pairs in the bulk. We expect our results to be helpful in constructing supersymmetric AdS_2 X S^2 perturbative string vacua, which enter in the near-horizon limit of extremal charged black holes. Although the generalized Breit...","downloadable_attachments":[{"id":84949761,"asset_id":77632669,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":37740253,"first_name":"Jan","last_name":"Troost","domain_name":"ens","page_name":"JanTroost","display_name":"Jan Troost","profile_url":"https://ens.academia.edu/JanTroost?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":333,"name":"Field Theory","url":"https://www.academia.edu/Documents/in/Field_Theory?f_ri=14024","nofollow":false},{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false},{"id":10598,"name":"String Theory","url":"https://www.academia.edu/Documents/in/String_Theory?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":80414,"name":"Mathematical 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In unified field theory all the objects are geometrical, for strings the Kalb-Ramond matter field is identical to the... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_34275324" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">It is argued that string theory predicts unified field theory rather than general relativity coupled to matter fields. In unified field theory all the objects are geometrical, for strings the Kalb-Ramond matter field is identical to the asymmetric part of the metric except that the fields contribute to different sides of the field equations. The dilaton is related to the object of non-metricity.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/34275324" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="87598c9c65c398e4c063fc96d7e488c0" rel="nofollow" data-download="{"attachment_id":54182346,"asset_id":34275324,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/54182346/download_file?st=MTczMjQyMzQ5Nyw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="346504" href="https://independent.academia.edu/MarkRoberts">Mark D Roberts</a><script data-card-contents-for-user="346504" type="text/json">{"id":346504,"first_name":"Mark","last_name":"Roberts","domain_name":"independent","page_name":"MarkRoberts","display_name":"Mark D Roberts","profile_url":"https://independent.academia.edu/MarkRoberts?f_ri=14024","photo":"https://0.academia-photos.com/346504/94133/161145/s65_mark.roberts.jpg"}</script></span></span></li><li class="js-paper-rank-work_34275324 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="34275324"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 34275324, container: ".js-paper-rank-work_34275324", }); 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Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":77311,"name":"Unified Field Theory","url":"https://www.academia.edu/Documents/in/Unified_Field_Theory?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_960546" data-work_id="960546" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/960546/The_ATLAS_experiment_at_the_CERN_large_hadron_collider">The ATLAS experiment at the CERN large hadron collider</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" 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class="InlineList-item-text" data-has-card-for-ri="118582" href="https://www.academia.edu/Documents/in/Physical_sciences">Physical sciences</a><script data-card-contents-for-ri="118582" type="text/json">{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=25050255]'), work: {"id":25050255,"title":"Non-planar master integrals for the production of two off-shell vector bosons in collisions of massless 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Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false},{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_71857373" data-work_id="71857373" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/71857373/The_Fundamental_Holographic_Uncertainty_Principle_and_its_Primary_Applications">The Fundamental Holographic Uncertainty Principle and its Primary Applications</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">The fundamental holographic principle is first proposed, then demonstrated in its validity and viability through a thought experiment and then finally derived. The Heisenberg uncertainty relations are shown to follow from this fundamental... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_71857373" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">The fundamental holographic principle is first proposed, then demonstrated in its validity and viability through a thought experiment and then finally derived. The Heisenberg uncertainty relations are shown to follow from this fundamental relation. The quantum blackhole entropy is then demonstrated using this holographic uncertainty relation along with the application of the Landauer’s principle for the thermodynamic erasure of a bit yielding a formula with a logarithmic correction. The blackhole entropy is found to be half the value normally delivered by any other method. So, it is proposed that there is a real relevant physical horizon at the twice the Schwarzschild radius dubbed the holographic information geometric horizon.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/71857373" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="48e8f8e119267b68a8c01af42989ae05" rel="nofollow" data-download="{"attachment_id":81032719,"asset_id":71857373,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/81032719/download_file?st=MTczMjQyMzQ5Nyw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="31668792" href="https://git.academia.edu/KoustubhKabe">Koustubh Kabe</a><script data-card-contents-for-user="31668792" type="text/json">{"id":31668792,"first_name":"Koustubh","last_name":"Kabe","domain_name":"git","page_name":"KoustubhKabe","display_name":"Koustubh Kabe","profile_url":"https://git.academia.edu/KoustubhKabe?f_ri=14024","photo":"https://0.academia-photos.com/31668792/9384076/10458470/s65_koustubh.kabe.jpg"}</script></span></span></li><li class="js-paper-rank-work_71857373 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="71857373"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 71857373, container: ".js-paper-rank-work_71857373", }); 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The Heisenberg uncertainty relations are shown to follow from this fundamental relation. The quantum blackhole entropy is then demonstrated using this holographic uncertainty relation along with the application of the Landauer’s principle for the thermodynamic erasure of a bit yielding a formula with a logarithmic correction. The blackhole entropy is found to be half the value normally delivered by any other method. So, it is proposed that there is a real relevant physical horizon at the twice the Schwarzschild radius dubbed the holographic information geometric horizon.","downloadable_attachments":[{"id":81032719,"asset_id":71857373,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":31668792,"first_name":"Koustubh","last_name":"Kabe","domain_name":"git","page_name":"KoustubhKabe","display_name":"Koustubh Kabe","profile_url":"https://git.academia.edu/KoustubhKabe?f_ri=14024","photo":"https://0.academia-photos.com/31668792/9384076/10458470/s65_koustubh.kabe.jpg"}],"research_interests":[{"id":504,"name":"Computational Physics","url":"https://www.academia.edu/Documents/in/Computational_Physics?f_ri=14024","nofollow":false},{"id":1246,"name":"Gravitation","url":"https://www.academia.edu/Documents/in/Gravitation?f_ri=14024","nofollow":false},{"id":3396,"name":"Foundations of Quantum Mechanics","url":"https://www.academia.edu/Documents/in/Foundations_of_Quantum_Mechanics?f_ri=14024","nofollow":false},{"id":3504,"name":"General Relativity","url":"https://www.academia.edu/Documents/in/General_Relativity?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024"},{"id":16682,"name":"Mathematical Modelling","url":"https://www.academia.edu/Documents/in/Mathematical_Modelling?f_ri=14024"},{"id":23179,"name":"Astrophysics","url":"https://www.academia.edu/Documents/in/Astrophysics?f_ri=14024"},{"id":28545,"name":"Loop Quantum Gravity","url":"https://www.academia.edu/Documents/in/Loop_Quantum_Gravity?f_ri=14024"},{"id":36265,"name":"Entropy","url":"https://www.academia.edu/Documents/in/Entropy?f_ri=14024"},{"id":47598,"name":"Cosmology","url":"https://www.academia.edu/Documents/in/Cosmology?f_ri=14024"},{"id":79394,"name":"Gravity","url":"https://www.academia.edu/Documents/in/Gravity?f_ri=14024"},{"id":126836,"name":"Blackhole Physics","url":"https://www.academia.edu/Documents/in/Blackhole_Physics?f_ri=14024"},{"id":192341,"name":"Blackholes","url":"https://www.academia.edu/Documents/in/Blackholes?f_ri=14024"},{"id":856293,"name":"Consequences from Heisenberg Uncertainty Relation","url":"https://www.academia.edu/Documents/in/Consequences_from_Heisenberg_Uncertainty_Relation?f_ri=14024"},{"id":1023356,"name":"Conditions of Uncertainty","url":"https://www.academia.edu/Documents/in/Conditions_of_Uncertainty?f_ri=14024"},{"id":1245467,"name":"Holographic Principle","url":"https://www.academia.edu/Documents/in/Holographic_Principle?f_ri=14024"},{"id":1325624,"name":"Geometrodynamics","url":"https://www.academia.edu/Documents/in/Geometrodynamics?f_ri=14024"},{"id":1372725,"name":"Geometrothermodynamics","url":"https://www.academia.edu/Documents/in/Geometrothermodynamics?f_ri=14024"},{"id":1404877,"name":"Logarithmic correction to BH entropy as Noether charge","url":"https://www.academia.edu/Documents/in/Logarithmic_correction_to_BH_entropy_as_Noether_charge?f_ri=14024"},{"id":1539232,"name":"Holographic Universe","url":"https://www.academia.edu/Documents/in/Holographic_Universe?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_69989448" data-work_id="69989448" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/69989448/Hamiltons_equations_in_a_non_associative_quantum_theory">Hamilton's equations in a non-associative quantum theory</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">A new non-associative algebra for the quantization of strongly interacting fields is proposed. The full set of quantum $(\pm)$associators for the product of three operators is offered. An algorithm for the calculation of some... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_69989448" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">A new non-associative algebra for the quantization of strongly interacting fields is proposed. The full set of quantum $(\pm)$associators for the product of three operators is offered. An algorithm for the calculation of some $(\pm)$associators for the product of some four operators is offered. The possible generalization of Hamilton&#39;s equations for a non-associative quantum theory is proposed. Some arguments are given that a non-associative quantum theory can be a fundamental unifying theory.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/69989448" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="c47371dbefbec9748b860de5bb107ff7" rel="nofollow" data-download="{"attachment_id":79882567,"asset_id":69989448,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/79882567/download_file?st=MTczMjQyMzQ5Nyw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="3431982" href="https://kaznu.academia.edu/VladimirDzhunushaliev">Vladimir Dzhunushaliev</a><script data-card-contents-for-user="3431982" type="text/json">{"id":3431982,"first_name":"Vladimir","last_name":"Dzhunushaliev","domain_name":"kaznu","page_name":"VladimirDzhunushaliev","display_name":"Vladimir Dzhunushaliev","profile_url":"https://kaznu.academia.edu/VladimirDzhunushaliev?f_ri=14024","photo":"https://0.academia-photos.com/3431982/46344940/35842215/s65_vladimir.dzhunushaliev.jpg"}</script></span></span></li><li class="js-paper-rank-work_69989448 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="69989448"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 69989448, container: ".js-paper-rank-work_69989448", }); 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$(".js-view-count[data-work-id=69989448]").text(description); $(".js-view-count-work_69989448").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_69989448").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="69989448"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">6</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="300" href="https://www.academia.edu/Documents/in/Mathematics">Mathematics</a>, <script data-card-contents-for-ri="300" type="text/json">{"id":300,"name":"Mathematics","url":"https://www.academia.edu/Documents/in/Mathematics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="337" href="https://www.academia.edu/Documents/in/Associative_Algebra">Associative Algebra</a>, <script data-card-contents-for-ri="337" type="text/json">{"id":337,"name":"Associative Algebra","url":"https://www.academia.edu/Documents/in/Associative_Algebra?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="498" href="https://www.academia.edu/Documents/in/Physics">Physics</a>, <script data-card-contents-for-ri="498" type="text/json">{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="518" href="https://www.academia.edu/Documents/in/Quantum_Physics">Quantum Physics</a><script data-card-contents-for-ri="518" type="text/json">{"id":518,"name":"Quantum Physics","url":"https://www.academia.edu/Documents/in/Quantum_Physics?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=69989448]'), work: {"id":69989448,"title":"Hamilton's equations in a non-associative quantum theory","created_at":"2022-01-29T20:00:19.307-08:00","url":"https://www.academia.edu/69989448/Hamiltons_equations_in_a_non_associative_quantum_theory?f_ri=14024","dom_id":"work_69989448","summary":"A new non-associative algebra for the quantization of strongly interacting fields is proposed. The full set of quantum $(\\pm)$associators for the product of three operators is offered. An algorithm for the calculation of some $(\\pm)$associators for the product of some four operators is offered. The possible generalization of Hamilton\u0026#39;s equations for a non-associative quantum theory is proposed. Some arguments are given that a non-associative quantum theory can be a fundamental unifying theory.","downloadable_attachments":[{"id":79882567,"asset_id":69989448,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":3431982,"first_name":"Vladimir","last_name":"Dzhunushaliev","domain_name":"kaznu","page_name":"VladimirDzhunushaliev","display_name":"Vladimir Dzhunushaliev","profile_url":"https://kaznu.academia.edu/VladimirDzhunushaliev?f_ri=14024","photo":"https://0.academia-photos.com/3431982/46344940/35842215/s65_vladimir.dzhunushaliev.jpg"}],"research_interests":[{"id":300,"name":"Mathematics","url":"https://www.academia.edu/Documents/in/Mathematics?f_ri=14024","nofollow":false},{"id":337,"name":"Associative Algebra","url":"https://www.academia.edu/Documents/in/Associative_Algebra?f_ri=14024","nofollow":false},{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false},{"id":518,"name":"Quantum Physics","url":"https://www.academia.edu/Documents/in/Quantum_Physics?f_ri=14024","nofollow":false},{"id":6811,"name":"Quantum Theory","url":"https://www.academia.edu/Documents/in/Quantum_Theory?f_ri=14024"},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_69323336" data-work_id="69323336" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/69323336/Conformal_invariant_strings_with_extrinsic_curvature_action">Conformal invariant strings with extrinsic curvature action</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We study a string theory which is exclusively based on extrinsic curvature action. It is a tensionless string theory because the action reduces to perimeter for the flat Wilson loop. We are able to solve and quantize this high-derivative... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_69323336" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We study a string theory which is exclusively based on extrinsic curvature action. It is a tensionless string theory because the action reduces to perimeter for the flat Wilson loop. We are able to solve and quantize this high-derivative nonlinear two-dimensional conformal field theory. The absence of conformal anomaly in quantum theory requires that the space-time should be 13-dimensional. We have found that all particles, with arbitrary large spin, are massless. This pure massless spectrum is consistent with the tensionless character of the theory and we speculate that it may describe unbroken phase of standard string theory.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/69323336" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="2de0745e29eb89202334999d1fa3f3e3" rel="nofollow" data-download="{"attachment_id":79463428,"asset_id":69323336,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/79463428/download_file?st=MTczMjQyMzQ5Nyw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="37957534" href="https://independent.academia.edu/GeorgeSavvidy">George Savvidy</a><script data-card-contents-for-user="37957534" type="text/json">{"id":37957534,"first_name":"George","last_name":"Savvidy","domain_name":"independent","page_name":"GeorgeSavvidy","display_name":"George Savvidy","profile_url":"https://independent.academia.edu/GeorgeSavvidy?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_69323336 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="69323336"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 69323336, container: ".js-paper-rank-work_69323336", }); 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$(".js-view-count[data-work-id=69323336]").text(description); $(".js-view-count-work_69323336").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_69323336").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="69323336"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">8</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="498" href="https://www.academia.edu/Documents/in/Physics">Physics</a>, <script data-card-contents-for-ri="498" type="text/json">{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="6811" href="https://www.academia.edu/Documents/in/Quantum_Theory">Quantum Theory</a>, <script data-card-contents-for-ri="6811" type="text/json">{"id":6811,"name":"Quantum Theory","url":"https://www.academia.edu/Documents/in/Quantum_Theory?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="10598" href="https://www.academia.edu/Documents/in/String_Theory">String Theory</a>, <script data-card-contents-for-ri="10598" type="text/json">{"id":10598,"name":"String Theory","url":"https://www.academia.edu/Documents/in/String_Theory?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a><script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=69323336]'), work: {"id":69323336,"title":"Conformal invariant strings with extrinsic curvature action","created_at":"2022-01-24T00:25:45.765-08:00","url":"https://www.academia.edu/69323336/Conformal_invariant_strings_with_extrinsic_curvature_action?f_ri=14024","dom_id":"work_69323336","summary":"We study a string theory which is exclusively based on extrinsic curvature action. It is a tensionless string theory because the action reduces to perimeter for the flat Wilson loop. We are able to solve and quantize this high-derivative nonlinear two-dimensional conformal field theory. The absence of conformal anomaly in quantum theory requires that the space-time should be 13-dimensional. We have found that all particles, with arbitrary large spin, are massless. This pure massless spectrum is consistent with the tensionless character of the theory and we speculate that it may describe unbroken phase of standard string theory.","downloadable_attachments":[{"id":79463428,"asset_id":69323336,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":37957534,"first_name":"George","last_name":"Savvidy","domain_name":"independent","page_name":"GeorgeSavvidy","display_name":"George Savvidy","profile_url":"https://independent.academia.edu/GeorgeSavvidy?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false},{"id":6811,"name":"Quantum Theory","url":"https://www.academia.edu/Documents/in/Quantum_Theory?f_ri=14024","nofollow":false},{"id":10598,"name":"String Theory","url":"https://www.academia.edu/Documents/in/String_Theory?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":154543,"name":"Space Time","url":"https://www.academia.edu/Documents/in/Space_Time?f_ri=14024"},{"id":154823,"name":"Conformal Field Theory","url":"https://www.academia.edu/Documents/in/Conformal_Field_Theory?f_ri=14024"},{"id":321836,"name":"Spectrum","url":"https://www.academia.edu/Documents/in/Spectrum?f_ri=14024"},{"id":2895246,"name":"Conformal Invariance","url":"https://www.academia.edu/Documents/in/Conformal_Invariance?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_55818363" data-work_id="55818363" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/55818363/Yukawa_couplings_and_masses_of_non_chiral_states_for_the_Standard_Model_on_D6_branes_on_T_6_mathbb_Z_6_prime_">Yukawa couplings and masses of non-chiral states for the Standard Model on D6-branes on $ {T^{{6}}}/\mathbb{Z}_{{6}}^{\prime } $</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/55818363" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="bda662adc5f87cc7fd168d2ef075dda7" rel="nofollow" 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data-card-contents-for-ri="80414" type="text/json">{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="118582" href="https://www.academia.edu/Documents/in/Physical_sciences">Physical sciences</a><script data-card-contents-for-ri="118582" type="text/json">{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=55818363]'), work: {"id":55818363,"title":"Yukawa couplings and masses of non-chiral states for the Standard Model on D6-branes on $ {T^{{6}}}/\\mathbb{Z}_{{6}}^{\\prime } $","created_at":"2021-10-05T23:02:57.834-07:00","url":"https://www.academia.edu/55818363/Yukawa_couplings_and_masses_of_non_chiral_states_for_the_Standard_Model_on_D6_branes_on_T_6_mathbb_Z_6_prime_?f_ri=14024","dom_id":"work_55818363","summary":null,"downloadable_attachments":[{"id":71508599,"asset_id":55818363,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":78383276,"first_name":"Gabriele","last_name":"Honecker","domain_name":"uni-mainz","page_name":"GabrieleHonecker","display_name":"Gabriele Honecker","profile_url":"https://uni-mainz.academia.edu/GabrieleHonecker?f_ri=14024","photo":"https://0.academia-photos.com/78383276/46799265/36053531/s65_gabriele.honecker.jpg"}],"research_interests":[{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false},{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_50112922" data-work_id="50112922" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/50112922/Applications_for_the_scalable_coherent_interface">Applications for the scalable coherent interface</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm 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data-has-card-for-ri="104336" href="https://www.academia.edu/Documents/in/Data_acquisition">Data acquisition</a><script data-card-contents-for-ri="104336" type="text/json">{"id":104336,"name":"Data acquisition","url":"https://www.academia.edu/Documents/in/Data_acquisition?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=50112922]'), work: {"id":50112922,"title":"Applications for the scalable coherent interface","created_at":"2021-07-20T14:16:08.232-07:00","url":"https://www.academia.edu/50112922/Applications_for_the_scalable_coherent_interface?f_ri=14024","dom_id":"work_50112922","summary":null,"downloadable_attachments":[{"id":68220227,"asset_id":50112922,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":7582568,"first_name":"David","last_name":"Gustavson","domain_name":"independent","page_name":"DavidGustavson","display_name":"David 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In the simple two flavor (ν µ , ν e) case, the probability that ν µ changes to ν e is expressed by P νµ→νe = sin 2... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_37169403" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Neutrino oscillation is a quantum mechanical phenomenon in which neutrino flavor changes spontaneously to another flavor. In the simple two flavor (ν µ , ν e) case, the probability that ν µ changes to ν e is expressed by P νµ→νe = sin 2 2θ sin 2 m 2 2 − m 2 1 4E ν L where E ν is the neutrino energy, L is the distance between the neutrino source and detector, m 1 and m 2 are the neutrino masses of the mass eigenstates and θ is the mixing angle between flavor eigenstates and mass eigenstates.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/37169403" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="d081face754d3c064d39c303e82b7eba" rel="nofollow" data-download="{"attachment_id":57120548,"asset_id":37169403,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/57120548/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="2792810" href="https://independentresearcher.academia.edu/DrJMAshfaqueAMIMAMInstP">Dr. J. 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In the simple two flavor (ν µ , ν e) case, the probability that ν µ changes to ν e is expressed by P νµ→νe = sin 2 2θ sin 2 m 2 2 − m 2 1 4E ν L where E ν is the neutrino energy, L is the distance between the neutrino source and detector, m 1 and m 2 are the neutrino masses of the mass eigenstates and θ is the mixing angle between flavor eigenstates and mass eigenstates.","downloadable_attachments":[{"id":57120548,"asset_id":37169403,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":2792810,"first_name":"Dr. J. M.","last_name":"Ashfaque (MInstP)","domain_name":"independentresearcher","page_name":"DrJMAshfaqueAMIMAMInstP","display_name":"Dr. J. M. 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The branching ratios of the singly... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_74397197" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Cabibbo-suppressed charm decays offer a good laboratory for studying weak interactions as they provide a unique window on the physics governing the decay-rate dynamics and CP violation. The branching ratios of the singly Cabibbo-suppressed decays of D0 meson are anomalous since the branching fraction of D0! m mÿ is observed to be suppressed relative to that of D0! K Kÿ by a factor of almost three [1], even though the phase space for the former is larger. The branching ratios of three-body decays of the D0 [2, 3] have larger uncertainties ...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/74397197" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="07464e1ea7d4bae3ca92d01589ff6565" rel="nofollow" data-download="{"attachment_id":82564633,"asset_id":74397197,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/82564633/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="135229858" href="https://independent.academia.edu/ZieglerVeronique">Veronique Ziegler</a><script data-card-contents-for-user="135229858" type="text/json">{"id":135229858,"first_name":"Veronique","last_name":"Ziegler","domain_name":"independent","page_name":"ZieglerVeronique","display_name":"Veronique Ziegler","profile_url":"https://independent.academia.edu/ZieglerVeronique?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_74397197 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="74397197"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 74397197, container: ".js-paper-rank-work_74397197", }); 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The branching ratios of three-body decays of the D0 [2, 3] have larger uncertainties ...","downloadable_attachments":[{"id":82564633,"asset_id":74397197,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":135229858,"first_name":"Veronique","last_name":"Ziegler","domain_name":"independent","page_name":"ZieglerVeronique","display_name":"Veronique Ziegler","profile_url":"https://independent.academia.edu/ZieglerVeronique?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false},{"id":518,"name":"Quantum Physics","url":"https://www.academia.edu/Documents/in/Quantum_Physics?f_ri=14024","nofollow":false},{"id":7936,"name":"Quantum Mechanics","url":"https://www.academia.edu/Documents/in/Quantum_Mechanics?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":235064,"name":"Time Reversal","url":"https://www.academia.edu/Documents/in/Time_Reversal?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_68772781" data-work_id="68772781" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/68772781/Black_hole_thermodynamics_and_massive_gravity">Black hole thermodynamics and massive gravity</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/68772781" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="2d9f28bc7ac28d716b674f17db4297ba" rel="nofollow" data-download="{"attachment_id":79130611,"asset_id":68772781,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/79130611/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="32034299" href="https://independent.academia.edu/FabioCapela">Fabio Capela</a><script data-card-contents-for-user="32034299" type="text/json">{"id":32034299,"first_name":"Fabio","last_name":"Capela","domain_name":"independent","page_name":"FabioCapela","display_name":"Fabio Capela","profile_url":"https://independent.academia.edu/FabioCapela?f_ri=14024","photo":"https://0.academia-photos.com/32034299/9548589/10636968/s65_fabio.capela.jpg"}</script></span></span></li><li class="js-paper-rank-work_68772781 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="68772781"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 68772781, container: ".js-paper-rank-work_68772781", }); 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D. Thesis we concentrate on the study of the extension of the AdS/CFT correspondence to theories with less supersymmetry. In particular, we search for the possibility of adding supersymmetric D-branes in type IIB supergravity... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_64177616" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">In this Ph. D. Thesis we concentrate on the study of the extension of the AdS/CFT correspondence to theories with less supersymmetry. In particular, we search for the possibility of adding supersymmetric D-branes in type IIB supergravity solutions which are dual to N=1 supersymmetric gauge theories in four dimensions. In the probe approximation we perform a systematic analysis of the possible supersymmetric D-brane configurations in backgrounds dual to N=1 superconformal field theories, firstly in the AdS_5xY^{p,q} solutions and then in their generalisation to the AdS_5xL^{a,b,c} backgrounds. Some checks of the correspondence between D-brane configurations and chiral operators of the dual gauge theory are performed. We also analyse the possible supersymmetric D5-brane configurations dual to defects (of codimension one and two) in N=1 SYM theory in the framework of the Maldacena-Nunez solution. Beyond the probe approximation, we develop techniques in order to take into account the ba...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/64177616" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="acc84b8aab73d50bf382d2b32abab48a" rel="nofollow" data-download="{"attachment_id":76333519,"asset_id":64177616,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/76333519/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="209761822" href="https://independent.academia.edu/FelipeCanoura">Felipe Canoura</a><script data-card-contents-for-user="209761822" type="text/json">{"id":209761822,"first_name":"Felipe","last_name":"Canoura","domain_name":"independent","page_name":"FelipeCanoura","display_name":"Felipe Canoura","profile_url":"https://independent.academia.edu/FelipeCanoura?f_ri=14024","photo":"https://0.academia-photos.com/209761822/69510379/57910839/s65_felipe.canoura.png"}</script></span></span></li><li class="js-paper-rank-work_64177616 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="64177616"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 64177616, container: ".js-paper-rank-work_64177616", }); 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D. Thesis we concentrate on the study of the extension of the AdS/CFT correspondence to theories with less supersymmetry. In particular, we search for the possibility of adding supersymmetric D-branes in type IIB supergravity solutions which are dual to N=1 supersymmetric gauge theories in four dimensions. In the probe approximation we perform a systematic analysis of the possible supersymmetric D-brane configurations in backgrounds dual to N=1 superconformal field theories, firstly in the AdS_5xY^{p,q} solutions and then in their generalisation to the AdS_5xL^{a,b,c} backgrounds. Some checks of the correspondence between D-brane configurations and chiral operators of the dual gauge theory are performed. We also analyse the possible supersymmetric D5-brane configurations dual to defects (of codimension one and two) in N=1 SYM theory in the framework of the Maldacena-Nunez solution. Beyond the probe approximation, we develop techniques in order to take into account the ba...","downloadable_attachments":[{"id":76333519,"asset_id":64177616,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":209761822,"first_name":"Felipe","last_name":"Canoura","domain_name":"independent","page_name":"FelipeCanoura","display_name":"Felipe Canoura","profile_url":"https://independent.academia.edu/FelipeCanoura?f_ri=14024","photo":"https://0.academia-photos.com/209761822/69510379/57910839/s65_felipe.canoura.png"}],"research_interests":[{"id":333,"name":"Field Theory","url":"https://www.academia.edu/Documents/in/Field_Theory?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":108262,"name":"Gauge theory","url":"https://www.academia.edu/Documents/in/Gauge_theory?f_ri=14024","nofollow":false},{"id":915258,"name":"Supersymmetric Gauge Theory","url":"https://www.academia.edu/Documents/in/Supersymmetric_Gauge_Theory?f_ri=14024","nofollow":false},{"id":3809690,"name":"Beta function","url":"https://www.academia.edu/Documents/in/Beta_function?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_21912968" data-work_id="21912968" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/21912968/Hot_and_dense_matter_in_quark_hadron_models">Hot and dense matter in quark-hadron models</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We present a general approach to incorporate hadronic as well as quark degrees of freedom in a unified approach. This approach implements the correct degrees of freedom at high as well as low temperatures and densities. An effective... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_21912968" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We present a general approach to incorporate hadronic as well as quark degrees of freedom in a unified approach. This approach implements the correct degrees of freedom at high as well as low temperatures and densities. An effective Polyakov loop field serves as the order parameter for deconfinement. We employ a well-tested hadronic flavor-SU(3) model based on a chirally symmetric formulation that reproduces properties of ground state nuclear matter and yields good descriptions of nuclei and hypernuclei. Excluded volume effects simulating the finite size of the hadrons drive the transition to quarks at high temperatures and densities. We study the phase structure of the model and the transition to the quark gluon plasma and compare results to lattice gauge calculations.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/21912968" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="ac5ec25747faedf29e1a811ab1788acd" rel="nofollow" data-download="{"attachment_id":42645384,"asset_id":21912968,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/42645384/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="43094364" href="https://uni-frankfurt.academia.edu/JanSteinheimer">Jan Steinheimer</a><script data-card-contents-for-user="43094364" type="text/json">{"id":43094364,"first_name":"Jan","last_name":"Steinheimer","domain_name":"uni-frankfurt","page_name":"JanSteinheimer","display_name":"Jan Steinheimer","profile_url":"https://uni-frankfurt.academia.edu/JanSteinheimer?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_21912968 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="21912968"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 21912968, container: ".js-paper-rank-work_21912968", }); 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This approach implements the correct degrees of freedom at high as well as low temperatures and densities. An effective Polyakov loop field serves as the order parameter for deconfinement. We employ a well-tested hadronic flavor-SU(3) model based on a chirally symmetric formulation that reproduces properties of ground state nuclear matter and yields good descriptions of nuclei and hypernuclei. Excluded volume effects simulating the finite size of the hadrons drive the transition to quarks at high temperatures and densities. We study the phase structure of the model and the transition to the quark gluon plasma and compare results to lattice gauge calculations.","downloadable_attachments":[{"id":42645384,"asset_id":21912968,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":43094364,"first_name":"Jan","last_name":"Steinheimer","domain_name":"uni-frankfurt","page_name":"JanSteinheimer","display_name":"Jan Steinheimer","profile_url":"https://uni-frankfurt.academia.edu/JanSteinheimer?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":6763,"name":"Quark Gluon Plasma","url":"https://www.academia.edu/Documents/in/Quark_Gluon_Plasma?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":960474,"name":"Order Parameter","url":"https://www.academia.edu/Documents/in/Order_Parameter?f_ri=14024","nofollow":false},{"id":1242198,"name":"Degree of Freedom","url":"https://www.academia.edu/Documents/in/Degree_of_Freedom?f_ri=14024","nofollow":false},{"id":2019381,"name":"Nuclear matter","url":"https://www.academia.edu/Documents/in/Nuclear_matter?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_47292352" data-work_id="47292352" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/47292352/Fermion_fermion_and_boson_boson_amplitudes_surprising_similarities">Fermion-fermion and boson-boson amplitudes: surprising similarities</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/47292352" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="8ebb722c6546488f90e96f60f67d9afa" rel="nofollow" data-download="{"attachment_id":66461860,"asset_id":47292352,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/66461860/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="56387296" href="https://uaz.academia.edu/ValeriyDvoeglazov">Valeriy Dvoeglazov</a><script data-card-contents-for-user="56387296" type="text/json">{"id":56387296,"first_name":"Valeriy","last_name":"Dvoeglazov","domain_name":"uaz","page_name":"ValeriyDvoeglazov","display_name":"Valeriy Dvoeglazov","profile_url":"https://uaz.academia.edu/ValeriyDvoeglazov?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_47292352 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="47292352"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 47292352, container: ".js-paper-rank-work_47292352", }); 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The present state of T symmetry tests is discussed with an... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_81177918" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">This article reports on the feasibility of testing of the symmetry under reversal in time in a purely leptonic system constituted by positronium atoms using the J-PET detector. The present state of T symmetry tests is discussed with an emphasis on the scarcely explored sector of leptonic systems. Two possible strategies of searching for manifestations of T violation in nonvanishing angular correlations of final state observables in the decay of metastable triplet states of positronium available with J-PET are proposed and discussed. Results of a pilot measurement with J-PET and assessment of its performance in reconstruction of three-photon decays are shown along with an analysis of its impact on the sensitivity of the detector for the determination of T-violation sensitive observables.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/81177918" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="50a437c1e81eba252588eaac77ebfd88" rel="nofollow" data-download="{"attachment_id":87313666,"asset_id":81177918,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/87313666/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="52873776" href="https://independent.academia.edu/PMoskal">Pawel Moskal</a><script data-card-contents-for-user="52873776" type="text/json">{"id":52873776,"first_name":"Pawel","last_name":"Moskal","domain_name":"independent","page_name":"PMoskal","display_name":"Pawel Moskal","profile_url":"https://independent.academia.edu/PMoskal?f_ri=14024","photo":"https://0.academia-photos.com/52873776/30541885/28292993/s65_pawel.moskal.jpg"}</script></span></span></li><li class="js-paper-rank-work_81177918 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="81177918"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 81177918, container: ".js-paper-rank-work_81177918", }); 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$(".js-view-count[data-work-id=81177918]").text(description); $(".js-view-count-work_81177918").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_81177918").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="81177918"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">4</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="498" href="https://www.academia.edu/Documents/in/Physics">Physics</a>, <script data-card-contents-for-ri="498" type="text/json">{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="80414" href="https://www.academia.edu/Documents/in/Mathematical_Sciences">Mathematical Sciences</a>, <script data-card-contents-for-ri="80414" type="text/json">{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="118582" href="https://www.academia.edu/Documents/in/Physical_sciences">Physical sciences</a><script data-card-contents-for-ri="118582" type="text/json">{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=81177918]'), work: {"id":81177918,"title":"Feasibility Study of the Time Reversal Symmetry Tests in Decay of Metastable Positronium Atoms with the J-PET Detector","created_at":"2022-06-10T09:28:02.655-07:00","url":"https://www.academia.edu/81177918/Feasibility_Study_of_the_Time_Reversal_Symmetry_Tests_in_Decay_of_Metastable_Positronium_Atoms_with_the_J_PET_Detector?f_ri=14024","dom_id":"work_81177918","summary":"This article reports on the feasibility of testing of the symmetry under reversal in time in a purely leptonic system constituted by positronium atoms using the J-PET detector. The present state of T symmetry tests is discussed with an emphasis on the scarcely explored sector of leptonic systems. Two possible strategies of searching for manifestations of T violation in nonvanishing angular correlations of final state observables in the decay of metastable triplet states of positronium available with J-PET are proposed and discussed. Results of a pilot measurement with J-PET and assessment of its performance in reconstruction of three-photon decays are shown along with an analysis of its impact on the sensitivity of the detector for the determination of T-violation sensitive observables.","downloadable_attachments":[{"id":87313666,"asset_id":81177918,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":52873776,"first_name":"Pawel","last_name":"Moskal","domain_name":"independent","page_name":"PMoskal","display_name":"Pawel Moskal","profile_url":"https://independent.academia.edu/PMoskal?f_ri=14024","photo":"https://0.academia-photos.com/52873776/30541885/28292993/s65_pawel.moskal.jpg"}],"research_interests":[{"id":498,"name":"Physics","url":"https://www.academia.edu/Documents/in/Physics?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false},{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_72273118" data-work_id="72273118" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/72273118/FIMP_and_Muon_g_2_in_a_U_1_L_%CE%BC_L_%CF%84_Model">FIMP and Muon (g-2) in a U(1)_L_μ-L_τ Model</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">The tightening of the constraints on the standard thermal WIMP scenario has forced physicists to propose alternative dark matter (DM) models. One of the most popular alternate explanations of the origin of DM is the non-thermal production... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_72273118" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">The tightening of the constraints on the standard thermal WIMP scenario has forced physicists to propose alternative dark matter (DM) models. One of the most popular alternate explanations of the origin of DM is the non-thermal production of DM via freeze-in. In this scenario the DM never attains thermal equilibrium with the thermal soup because of its feeble coupling strength (∼ 10^-12) with the other particles in the thermal bath and is generally called the Feebly Interacting Massive Particle (FIMP). In this work, we present a gauged U(1)_L_μ-L_τ extension of the Standard Model (SM) which has a scalar FIMP DM candidate and can consistently explain the DM relic density bound. In addition, the spontaneous breaking of the U(1)_L_μ-L_τ gauge symmetry gives an extra massive neutral gauge boson Z_μτ which can explain the muon (g-2) data through its additional one-loop contribution to the process. Lastly, presence of three right-handed neutrinos enable the model to successfully explain t...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/72273118" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="a4c9870bd16108cd94ac2e9de8ae5e6b" rel="nofollow" data-download="{"attachment_id":81265489,"asset_id":72273118,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/81265489/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="167396243" href="https://independent.academia.edu/AnirbanBiswas48">Anirban Biswas</a><script data-card-contents-for-user="167396243" type="text/json">{"id":167396243,"first_name":"Anirban","last_name":"Biswas","domain_name":"independent","page_name":"AnirbanBiswas48","display_name":"Anirban Biswas","profile_url":"https://independent.academia.edu/AnirbanBiswas48?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_72273118 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="72273118"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 72273118, container: ".js-paper-rank-work_72273118", }); 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$(".js-view-count[data-work-id=72273118]").text(description); $(".js-view-count-work_72273118").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_72273118").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="72273118"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">3</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="80414" href="https://www.academia.edu/Documents/in/Mathematical_Sciences">Mathematical Sciences</a>, <script data-card-contents-for-ri="80414" type="text/json">{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="118582" href="https://www.academia.edu/Documents/in/Physical_sciences">Physical sciences</a><script data-card-contents-for-ri="118582" type="text/json">{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=72273118]'), work: {"id":72273118,"title":"FIMP and Muon (g-2) in a U(1)_L_μ-L_τ Model","created_at":"2022-02-22T18:58:05.667-08:00","url":"https://www.academia.edu/72273118/FIMP_and_Muon_g_2_in_a_U_1_L_%CE%BC_L_%CF%84_Model?f_ri=14024","dom_id":"work_72273118","summary":"The tightening of the constraints on the standard thermal WIMP scenario has forced physicists to propose alternative dark matter (DM) models. One of the most popular alternate explanations of the origin of DM is the non-thermal production of DM via freeze-in. In this scenario the DM never attains thermal equilibrium with the thermal soup because of its feeble coupling strength (∼ 10^-12) with the other particles in the thermal bath and is generally called the Feebly Interacting Massive Particle (FIMP). In this work, we present a gauged U(1)_L_μ-L_τ extension of the Standard Model (SM) which has a scalar FIMP DM candidate and can consistently explain the DM relic density bound. In addition, the spontaneous breaking of the U(1)_L_μ-L_τ gauge symmetry gives an extra massive neutral gauge boson Z_μτ which can explain the muon (g-2) data through its additional one-loop contribution to the process. Lastly, presence of three right-handed neutrinos enable the model to successfully explain t...","downloadable_attachments":[{"id":81265489,"asset_id":72273118,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":167396243,"first_name":"Anirban","last_name":"Biswas","domain_name":"independent","page_name":"AnirbanBiswas48","display_name":"Anirban Biswas","profile_url":"https://independent.academia.edu/AnirbanBiswas48?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false},{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_64294138" data-work_id="64294138" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/64294138/Noncommutative_Finsler_Geometry_Gauge_Fields_and_Gravity">Noncommutative Finsler Geometry, Gauge Fields and Gravity</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">AbstractThe work extends the A. Connes’ noncommutative geometry to spaces withgeneric local anisotropy. We apply the E. Cartan’s anholonomic frame approachto geometry models and physical theories and develop the nonlinear... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_64294138" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">AbstractThe work extends the A. Connes’ noncommutative geometry to spaces withgeneric local anisotropy. We apply the E. Cartan’s anholonomic frame approachto geometry models and physical theories and develop the nonlinear connectionformalism for projective modulespaces. Examples of noncommutative generationof anholonomic Riemann, Finsler and Lagrange spaces are analyzed. We alsopresent a research on noncommutative Finsler–gauge theories, generalized Finslergravity and anholonomic (pseudo) Riemann geometry which appear naturally ifanholonomic frames (vierbeins) are deﬁned in the context of string/M–theoryand extra dimension Riemann gravity..Pacs: 02.40.Gh, 02.40.-k, 04.50.+hMSC numbers: 83D05, 46L87, 58B34, 58B20, 53B40, 53C07 Contents 1 Introduction 22 Commutative and Noncommutative Spaces 42.1 Algebras of functions and (non) commutative spaces . . . . . . . . . . . 52.2 Commutative spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82.3 Noncommutative spaces . . . . . ....</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/64294138" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="80a311a4b2e796f5a5d6b54aaff8f666" rel="nofollow" data-download="{"attachment_id":76394507,"asset_id":64294138,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/76394507/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="7910585" href="https://independent.academia.edu/VacaruSergiu">Sergiu Vacaru</a><script data-card-contents-for-user="7910585" type="text/json">{"id":7910585,"first_name":"Sergiu","last_name":"Vacaru","domain_name":"independent","page_name":"VacaruSergiu","display_name":"Sergiu Vacaru","profile_url":"https://independent.academia.edu/VacaruSergiu?f_ri=14024","photo":"https://0.academia-photos.com/7910585/2848048/18283457/s65_sergiu.vacaru.jpg"}</script></span></span></li><li class="js-paper-rank-work_64294138 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="64294138"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 64294138, container: ".js-paper-rank-work_64294138", }); });</script></li><li class="js-percentile-work_64294138 InlineList-item InlineList-item--bordered hidden u-tcGrayDark"><span class="percentile-widget hidden"><span class="u-mr2x percentile-widget" style="display: none">•</span><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 64294138; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-percentile-work_64294138"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></li><li class="js-view-count-work_64294138 InlineList-item InlineList-item--bordered hidden"><div><span><span class="js-view-count view-count u-mr2x" data-work-id="64294138"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 64294138; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=64294138]").text(description); $(".js-view-count-work_64294138").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_64294138").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="64294138"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">9</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="318" href="https://www.academia.edu/Documents/in/Mathematical_Physics">Mathematical Physics</a>, <script data-card-contents-for-ri="318" type="text/json">{"id":318,"name":"Mathematical Physics","url":"https://www.academia.edu/Documents/in/Mathematical_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="6813" href="https://www.academia.edu/Documents/in/Quantum_Cosmology">Quantum Cosmology</a>, <script data-card-contents-for-ri="6813" type="text/json">{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14348" href="https://www.academia.edu/Documents/in/Differential_Geometry">Differential Geometry</a><script data-card-contents-for-ri="14348" type="text/json">{"id":14348,"name":"Differential Geometry","url":"https://www.academia.edu/Documents/in/Differential_Geometry?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=64294138]'), work: {"id":64294138,"title":"Noncommutative Finsler Geometry, Gauge Fields and Gravity","created_at":"2021-12-15T06:30:57.225-08:00","url":"https://www.academia.edu/64294138/Noncommutative_Finsler_Geometry_Gauge_Fields_and_Gravity?f_ri=14024","dom_id":"work_64294138","summary":"AbstractThe work extends the A. Connes’ noncommutative geometry to spaces withgeneric local anisotropy. We apply the E. Cartan’s anholonomic frame approachto geometry models and physical theories and develop the nonlinear connectionformalism for projective modulespaces. Examples of noncommutative generationof anholonomic Riemann, Finsler and Lagrange spaces are analyzed. We alsopresent a research on noncommutative Finsler–gauge theories, generalized Finslergravity and anholonomic (pseudo) Riemann geometry which appear naturally ifanholonomic frames (vierbeins) are deﬁned in the context of string/M–theoryand extra dimension Riemann gravity..Pacs: 02.40.Gh, 02.40.-k, 04.50.+hMSC numbers: 83D05, 46L87, 58B34, 58B20, 53B40, 53C07 Contents 1 Introduction 22 Commutative and Noncommutative Spaces 42.1 Algebras of functions and (non) commutative spaces . . . . . . . . . . . 52.2 Commutative spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82.3 Noncommutative spaces . . . . . ....","downloadable_attachments":[{"id":76394507,"asset_id":64294138,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":7910585,"first_name":"Sergiu","last_name":"Vacaru","domain_name":"independent","page_name":"VacaruSergiu","display_name":"Sergiu Vacaru","profile_url":"https://independent.academia.edu/VacaruSergiu?f_ri=14024","photo":"https://0.academia-photos.com/7910585/2848048/18283457/s65_sergiu.vacaru.jpg"}],"research_interests":[{"id":318,"name":"Mathematical Physics","url":"https://www.academia.edu/Documents/in/Mathematical_Physics?f_ri=14024","nofollow":false},{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":14348,"name":"Differential Geometry","url":"https://www.academia.edu/Documents/in/Differential_Geometry?f_ri=14024","nofollow":false},{"id":51108,"name":"Noncommutative Geometry","url":"https://www.academia.edu/Documents/in/Noncommutative_Geometry?f_ri=14024"},{"id":61108,"name":"Geometric model","url":"https://www.academia.edu/Documents/in/Geometric_model?f_ri=14024"},{"id":108262,"name":"Gauge theory","url":"https://www.academia.edu/Documents/in/Gauge_theory?f_ri=14024"},{"id":403158,"name":"Gauge Field","url":"https://www.academia.edu/Documents/in/Gauge_Field?f_ri=14024"},{"id":2724088,"name":"M-projective module","url":"https://www.academia.edu/Documents/in/M-projective_module?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_51130476" data-work_id="51130476" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/51130476/A_Spiral_Structure_for_Elementary_Particles">A Spiral Structure for Elementary Particles</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">In this paper we have tried to deduce the possible origin of particle and evolution of their intrinsic properties through spiral dynamics. We consider some of the observations which include exponential mass function of particles following... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_51130476" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">In this paper we have tried to deduce the possible origin of particle and evolution of their intrinsic properties through spiral dynamics. We consider some of the observations which include exponential mass function of particles following a sequence when fitted on logarithmic potential spiral, inwardly rotating spiral dynamics in Reaction-Diffusion System, the separation of Electron’s Spin-Charge-Orbit into quasi-particles. The paper brings a picture of particles and their Anti Particles in spiral form and explains how the difference in structure varies their properties. It also explains the effects on particles in Accelerator deduced through spiral dynamics.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/51130476" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="0823f11e972331421e2a6352c1427ef7" rel="nofollow" data-download="{"attachment_id":68972747,"asset_id":51130476,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/68972747/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="186600825" href="https://independent.academia.edu/SURAJKUMAR1478">SURAJ KUMAR</a><script data-card-contents-for-user="186600825" type="text/json">{"id":186600825,"first_name":"SURAJ","last_name":"KUMAR","domain_name":"independent","page_name":"SURAJKUMAR1478","display_name":"SURAJ KUMAR","profile_url":"https://independent.academia.edu/SURAJKUMAR1478?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_51130476 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="51130476"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 51130476, container: ".js-paper-rank-work_51130476", }); 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We consider some of the observations which include exponential mass function of particles following a sequence when fitted on logarithmic potential spiral, inwardly rotating spiral dynamics in Reaction-Diffusion System, the separation of Electron’s Spin-Charge-Orbit into quasi-particles. The paper brings a picture of particles and their Anti Particles in spiral form and explains how the difference in structure varies their properties. It also explains the effects on particles in Accelerator deduced through spiral dynamics.","downloadable_attachments":[{"id":68972747,"asset_id":51130476,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":186600825,"first_name":"SURAJ","last_name":"KUMAR","domain_name":"independent","page_name":"SURAJKUMAR1478","display_name":"SURAJ KUMAR","profile_url":"https://independent.academia.edu/SURAJKUMAR1478?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":54,"name":"Engineering Physics","url":"https://www.academia.edu/Documents/in/Engineering_Physics?f_ri=14024","nofollow":false},{"id":305,"name":"Applied Mathematics","url":"https://www.academia.edu/Documents/in/Applied_Mathematics?f_ri=14024","nofollow":false},{"id":504,"name":"Computational Physics","url":"https://www.academia.edu/Documents/in/Computational_Physics?f_ri=14024","nofollow":false},{"id":505,"name":"Condensed Matter Physics","url":"https://www.academia.edu/Documents/in/Condensed_Matter_Physics?f_ri=14024","nofollow":false},{"id":508,"name":"Elementary Particle Physics","url":"https://www.academia.edu/Documents/in/Elementary_Particle_Physics?f_ri=14024"},{"id":3396,"name":"Foundations of Quantum Mechanics","url":"https://www.academia.edu/Documents/in/Foundations_of_Quantum_Mechanics?f_ri=14024"},{"id":4818,"name":"Dark Matter","url":"https://www.academia.edu/Documents/in/Dark_Matter?f_ri=14024"},{"id":9138,"name":"Applied Physics","url":"https://www.academia.edu/Documents/in/Applied_Physics?f_ri=14024"},{"id":12553,"name":"History of Physics","url":"https://www.academia.edu/Documents/in/History_of_Physics?f_ri=14024"},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024"},{"id":16620,"name":"Dark Energy","url":"https://www.academia.edu/Documents/in/Dark_Energy?f_ri=14024"},{"id":18996,"name":"Experimental Physics","url":"https://www.academia.edu/Documents/in/Experimental_Physics?f_ri=14024"},{"id":25955,"name":"Emergent Quantum Gravity","url":"https://www.academia.edu/Documents/in/Emergent_Quantum_Gravity?f_ri=14024"},{"id":28545,"name":"Loop Quantum Gravity","url":"https://www.academia.edu/Documents/in/Loop_Quantum_Gravity?f_ri=14024"},{"id":46820,"name":"CERN Experiment","url":"https://www.academia.edu/Documents/in/CERN_Experiment?f_ri=14024"},{"id":51604,"name":"Mathematic","url":"https://www.academia.edu/Documents/in/Mathematic?f_ri=14024"},{"id":65989,"name":"Grand Unification","url":"https://www.academia.edu/Documents/in/Grand_Unification?f_ri=14024"},{"id":97703,"name":"Mathematical Methods of Physics","url":"https://www.academia.edu/Documents/in/Mathematical_Methods_of_Physics?f_ri=14024"},{"id":203777,"name":"Intrinsic","url":"https://www.academia.edu/Documents/in/Intrinsic?f_ri=14024"},{"id":253738,"name":"Gravity Waves","url":"https://www.academia.edu/Documents/in/Gravity_Waves?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_38125424" data-work_id="38125424" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/38125424/Simulation_of_Space_Shuttle_neutron_measurements_with_FLUKA">Simulation of Space Shuttle neutron measurements with FLUKA</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/38125424" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa 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itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="2729790" href="https://independent.academia.edu/FedericoCarminati">Federico Carminati</a><script data-card-contents-for-user="2729790" type="text/json">{"id":2729790,"first_name":"Federico","last_name":"Carminati","domain_name":"independent","page_name":"FedericoCarminati","display_name":"Federico Carminati","profile_url":"https://independent.academia.edu/FedericoCarminati?f_ri=14024","photo":"https://0.academia-photos.com/2729790/881238/1100425/s65_federico.carminati.jpg"}</script></span></span></li><li class="js-paper-rank-work_38125424 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="38125424"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 38125424, container: ".js-paper-rank-work_38125424", }); });</script></li><li 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var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=38125424]").text(description); $(".js-view-count-work_38125424").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_38125424").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="38125424"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">16</a>  </div><span class="InlineList-item-text u-textTruncate u-pl10x"><a class="InlineList-item-text" data-has-card-for-ri="406" href="https://www.academia.edu/Documents/in/Geology">Geology</a>, <script data-card-contents-for-ri="406" type="text/json">{"id":406,"name":"Geology","url":"https://www.academia.edu/Documents/in/Geology?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="10032" href="https://www.academia.edu/Documents/in/Radiation_Protection">Radiation Protection</a>, <script data-card-contents-for-ri="10032" type="text/json">{"id":10032,"name":"Radiation Protection","url":"https://www.academia.edu/Documents/in/Radiation_Protection?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="22998" href="https://www.academia.edu/Documents/in/Gamma_Rays">Gamma Rays</a><script data-card-contents-for-ri="22998" type="text/json">{"id":22998,"name":"Gamma 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Carminati","profile_url":"https://independent.academia.edu/FedericoCarminati?f_ri=14024","photo":"https://0.academia-photos.com/2729790/881238/1100425/s65_federico.carminati.jpg"}],"research_interests":[{"id":406,"name":"Geology","url":"https://www.academia.edu/Documents/in/Geology?f_ri=14024","nofollow":false},{"id":10032,"name":"Radiation Protection","url":"https://www.academia.edu/Documents/in/Radiation_Protection?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":22998,"name":"Gamma Rays","url":"https://www.academia.edu/Documents/in/Gamma_Rays?f_ri=14024","nofollow":false},{"id":53293,"name":"Software","url":"https://www.academia.edu/Documents/in/Software?f_ri=14024"},{"id":55258,"name":"Aluminum","url":"https://www.academia.edu/Documents/in/Aluminum?f_ri=14024"},{"id":66244,"name":"Space flight","url":"https://www.academia.edu/Documents/in/Space_flight?f_ri=14024"},{"id":69542,"name":"Computer Simulation","url":"https://www.academia.edu/Documents/in/Computer_Simulation?f_ri=14024"},{"id":138127,"name":"Radiation Measurements","url":"https://www.academia.edu/Documents/in/Radiation_Measurements?f_ri=14024"},{"id":235205,"name":"Neutrons","url":"https://www.academia.edu/Documents/in/Neutrons?f_ri=14024"},{"id":343667,"name":"Theoretical Models","url":"https://www.academia.edu/Documents/in/Theoretical_Models?f_ri=14024"},{"id":404000,"name":"Cross Section","url":"https://www.academia.edu/Documents/in/Cross_Section?f_ri=14024"},{"id":820041,"name":"Spacecraft","url":"https://www.academia.edu/Documents/in/Spacecraft?f_ri=14024"},{"id":984615,"name":"Cosmic Radiation","url":"https://www.academia.edu/Documents/in/Cosmic_Radiation?f_ri=14024"},{"id":1208793,"name":"Protons","url":"https://www.academia.edu/Documents/in/Protons?f_ri=14024"},{"id":1333436,"name":"Monte Carlo Method","url":"https://www.academia.edu/Documents/in/Monte_Carlo_Method?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_33105027 coauthored" data-work_id="33105027" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/33105027/Conformity_Analysis_Between_Experimental_and_Theoretical_Data_in_the_Study_Collisions_of_Relativistic_Heavy_Ion_The_Case_Space">Conformity Analysis Between Experimental and Theoretical Data in the Study Collisions of Relativistic Heavy Ion (The Case  -Space</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We applied the wavelet methodology to study the results of the chaotic behavior of the production of particles in relativistic collisions of heavy ions. We use wavelet coherence to analyze the correspondence between theoretical and... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_33105027" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We applied the wavelet methodology to study the results of the chaotic behavior of the production of particles in relativistic collisions of heavy ions. We use wavelet coherence to analyze the correspondence between theoretical and experimental data. We examined the 1-D phase space of variable (the case -space). We also compared the wavelet coherence values for -space and -space. It was also shown that the values of the wavelet of coherence depend on the values of the parameters p and q. We discussed our new results for the comparison purpose and findings were in the good agreements.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/33105027" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="e278d0db3f57847a2006b1bca26616aa" rel="nofollow" data-download="{"attachment_id":53201489,"asset_id":33105027,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/53201489/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="21046478" href="https://uog-gy.academia.edu/MohammadAyazAhmad">Mohammad Ayaz Ahmad</a><script data-card-contents-for-user="21046478" type="text/json">{"id":21046478,"first_name":"Mohammad Ayaz","last_name":"Ahmad","domain_name":"uog-gy","page_name":"MohammadAyazAhmad","display_name":"Mohammad Ayaz Ahmad","profile_url":"https://uog-gy.academia.edu/MohammadAyazAhmad?f_ri=14024","photo":"https://0.academia-photos.com/21046478/5809954/6602100/s65_mohammad_ayaz.ahmad.jpg"}</script></span></span><span class="u-displayInlineBlock InlineList-item-text"> and <span class="u-textDecorationUnderline u-clickable InlineList-item-text js-work-more-authors-33105027">+1</span><div class="hidden js-additional-users-33105027"><div><span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a href="https://independent.academia.edu/VyacheslavLyashenko">Vyacheslav Lyashenko</a></span></div></div></span><script>(function(){ var popoverSettings = { el: $('.js-work-more-authors-33105027'), placement: 'bottom', hide_delay: 200, html: true, content: function(){ return $('.js-additional-users-33105027').html(); 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class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/18781907/MHV_Lagrangian_for_N_4_super_Yang_Mills">MHV Lagrangian for N = 4 super Yang-Mills</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">Here we formulate two field redefinitions for N = 4 Super Yang-Mills in light cone superspace that generates only MHV vertices in the new Lagrangian. After careful consideration of the S-matrix equivalence theorem, we see that only the... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_18781907" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Here we formulate two field redefinitions for N = 4 Super Yang-Mills in light cone superspace that generates only MHV vertices in the new Lagrangian. After careful consideration of the S-matrix equivalence theorem, we see that only the canonical transformation gives the MHV Lagrangian that would correspond to the CSW expansion. 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Giveon, Kutasov and Seiberg (hep-th/9806194); 2. Hemming, Keski-Vakkuri (hep-th/0110252); Maldacena, Ooguri (hep-th/0001053)... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_68879242" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">The main purpose of the report is to provide some argumentation that three seemingly distinct approaches of 1. Giveon, Kutasov and Seiberg (hep-th/9806194); 2. Hemming, Keski-Vakkuri (hep-th/0110252); Maldacena, Ooguri (hep-th/0001053) and 3. I. Bars (hep-th/9503205) can be investigated by applying the mathematical methods of integral geometry on the Lobachevsky plane, developed previously by Gel&#39;fand, Graev and Vilenkin. All these methods can be used for finding the transformations, leaving the Kac-Moody and Virasoro algebras invariant. The near-distance limit of the Conformal Field Theory of the SL(2, R) WZW model of strings on an ADS3 background can also be interpreted in terms of the Lobachevsky Geometry : the non - euclidean distance is conserved and the Lobachevsky formulae for the angle of parallelism is recovered. Some preliminary technique from integral geometry for inverting the modified integral representation for the Kac- Moody algebra has been demonstrated.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/68879242" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="c63320606073ce1a48a4271b0d68b8ea" rel="nofollow" data-download="{"attachment_id":79194590,"asset_id":68879242,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/79194590/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="59930115" href="https://independent.academia.edu/BogdanDimitrov1">Bogdan Dimitrov</a><script data-card-contents-for-user="59930115" type="text/json">{"id":59930115,"first_name":"Bogdan","last_name":"Dimitrov","domain_name":"independent","page_name":"BogdanDimitrov1","display_name":"Bogdan Dimitrov","profile_url":"https://independent.academia.edu/BogdanDimitrov1?f_ri=14024","photo":"https://0.academia-photos.com/59930115/101263900/90418926/s65_bogdan.dimitrov.png"}</script></span></span></li><li class="js-paper-rank-work_68879242 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="68879242"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 68879242, container: ".js-paper-rank-work_68879242", }); 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$(".js-view-count[data-work-id=68879242]").text(description); $(".js-view-count-work_68879242").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_68879242").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="68879242"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">5</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="6813" href="https://www.academia.edu/Documents/in/Quantum_Cosmology">Quantum Cosmology</a>, <script data-card-contents-for-ri="6813" type="text/json">{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="154823" href="https://www.academia.edu/Documents/in/Conformal_Field_Theory">Conformal Field Theory</a>, <script data-card-contents-for-ri="154823" type="text/json">{"id":154823,"name":"Conformal Field Theory","url":"https://www.academia.edu/Documents/in/Conformal_Field_Theory?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="1555351" href="https://www.academia.edu/Documents/in/Euclidean_Distance">Euclidean Distance</a><script data-card-contents-for-ri="1555351" type="text/json">{"id":1555351,"name":"Euclidean Distance","url":"https://www.academia.edu/Documents/in/Euclidean_Distance?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=68879242]'), work: {"id":68879242,"title":"Integral Geometry on the Lobachevsky Plane and the Conformal Wess-Zumino-Witten Model of Strings on an ADS3 Background","created_at":"2022-01-20T13:15:11.298-08:00","url":"https://www.academia.edu/68879242/Integral_Geometry_on_the_Lobachevsky_Plane_and_the_Conformal_Wess_Zumino_Witten_Model_of_Strings_on_an_ADS3_Background?f_ri=14024","dom_id":"work_68879242","summary":"The main purpose of the report is to provide some argumentation that three seemingly distinct approaches of 1. Giveon, Kutasov and Seiberg (hep-th/9806194); 2. Hemming, Keski-Vakkuri (hep-th/0110252); Maldacena, Ooguri (hep-th/0001053) and 3. I. Bars (hep-th/9503205) can be investigated by applying the mathematical methods of integral geometry on the Lobachevsky plane, developed previously by Gel\u0026#39;fand, Graev and Vilenkin. All these methods can be used for finding the transformations, leaving the Kac-Moody and Virasoro algebras invariant. The near-distance limit of the Conformal Field Theory of the SL(2, R) WZW model of strings on an ADS3 background can also be interpreted in terms of the Lobachevsky Geometry : the non - euclidean distance is conserved and the Lobachevsky formulae for the angle of parallelism is recovered. Some preliminary technique from integral geometry for inverting the modified integral representation for the Kac- Moody algebra has been demonstrated.","downloadable_attachments":[{"id":79194590,"asset_id":68879242,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":59930115,"first_name":"Bogdan","last_name":"Dimitrov","domain_name":"independent","page_name":"BogdanDimitrov1","display_name":"Bogdan Dimitrov","profile_url":"https://independent.academia.edu/BogdanDimitrov1?f_ri=14024","photo":"https://0.academia-photos.com/59930115/101263900/90418926/s65_bogdan.dimitrov.png"}],"research_interests":[{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":154823,"name":"Conformal Field Theory","url":"https://www.academia.edu/Documents/in/Conformal_Field_Theory?f_ri=14024","nofollow":false},{"id":1555351,"name":"Euclidean Distance","url":"https://www.academia.edu/Documents/in/Euclidean_Distance?f_ri=14024","nofollow":false},{"id":2568297,"name":"Virasoro algebra","url":"https://www.academia.edu/Documents/in/Virasoro_algebra?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_48429717" data-work_id="48429717" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/48429717/Photoproduction_at_collider_energies_from_RHIC_and_HERA_to_the_LHC">Photoproduction at collider energies: from RHIC and HERA to the LHC</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">We present the mini-proceedings of the workshop on ``Photoproduction at collider energies: from RHIC and HERA to the LHC&#39;&#39; held at the European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*, Trento)... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_48429717" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">We present the mini-proceedings of the workshop on ``Photoproduction at collider energies: from RHIC and HERA to the LHC&#39;&#39; held at the European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*, Trento) from January 15 to 19, 2007. The workshop gathered both theorists and experimentalists to discuss the current status of investigations of high-energy photon-induced processes at</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/48429717" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="ec4ae63e5d9eff6f75dc0686351b4c36" rel="nofollow" data-download="{"attachment_id":67046128,"asset_id":48429717,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/67046128/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="39141965" href="https://independent.academia.edu/BrodskyStanley">Stanley Brodsky</a><script data-card-contents-for-user="39141965" type="text/json">{"id":39141965,"first_name":"Stanley","last_name":"Brodsky","domain_name":"independent","page_name":"BrodskyStanley","display_name":"Stanley Brodsky","profile_url":"https://independent.academia.edu/BrodskyStanley?f_ri=14024","photo":"https://0.academia-photos.com/39141965/70804958/59234057/s65_stanley.brodsky.jpg"}</script></span></span></li><li class="js-paper-rank-work_48429717 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="48429717"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 48429717, container: ".js-paper-rank-work_48429717", }); 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held at the European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*, Trento) from January 15 to 19, 2007. 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energy","url":"https://www.academia.edu/Documents/in/High_energy?f_ri=14024","nofollow":false},{"id":1799006,"name":"Hadron Colliders","url":"https://www.academia.edu/Documents/in/Hadron_Colliders?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_7572268" data-work_id="7572268" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/7572268/Ice_free_cryopreservation_of_mouse_embryos_at_196_C_by_vitrification">Ice-free cryopreservation of mouse embryos at −196 °C by vitrification</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue 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The interactions and dynamics of these 1-form and Grassmann valued parts of an E8 superconnection are described by the curvature and action over a four dimensional base manifold.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/67413038" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="30ffbb35ab4e5c2267ca40eee54d15c7" rel="nofollow" data-download="{"attachment_id":78238976,"asset_id":67413038,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/78238976/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="32032314" href="https://independent.academia.edu/LisiGarrett">Garrett Lisi</a><script data-card-contents-for-user="32032314" type="text/json">{"id":32032314,"first_name":"Garrett","last_name":"Lisi","domain_name":"independent","page_name":"LisiGarrett","display_name":"Garrett Lisi","profile_url":"https://independent.academia.edu/LisiGarrett?f_ri=14024","photo":"https://gravatar.com/avatar/08432fb4d3f62de737be8165a8848072?s=65"}</script></span></span></li><li class="js-paper-rank-work_67413038 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="67413038"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 67413038, container: ".js-paper-rank-work_67413038", }); 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A non-compact real form of the E8 Lie algebra has G2 and F4 subalgebras which break down to strong su(3), electroweak su(2) x u(1), gravitational so(3,1), the frame-Higgs, and three generations of fermions related by triality. The interactions and dynamics of these 1-form and Grassmann valued parts of an E8 superconnection are described by the curvature and action over a four dimensional base manifold.","downloadable_attachments":[{"id":78238976,"asset_id":67413038,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":32032314,"first_name":"Garrett","last_name":"Lisi","domain_name":"independent","page_name":"LisiGarrett","display_name":"Garrett Lisi","profile_url":"https://independent.academia.edu/LisiGarrett?f_ri=14024","photo":"https://gravatar.com/avatar/08432fb4d3f62de737be8165a8848072?s=65"}],"research_interests":[{"id":336,"name":"Lie Algebra","url":"https://www.academia.edu/Documents/in/Lie_Algebra?f_ri=14024","nofollow":false},{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":130616,"name":"Standard Model","url":"https://www.academia.edu/Documents/in/Standard_Model?f_ri=14024","nofollow":false},{"id":3193313,"name":"arXiv","url":"https://www.academia.edu/Documents/in/arXiv?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_62101608" data-work_id="62101608" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/62101608/TMVA_Toolkit_for_Multivariate_Data_Analysis">TMVA-Toolkit for Multivariate Data Analysis</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized"> In high-energy physics, with the search for ever smaller signals in ever larger data sets, it has become essential to extract a maximum of the available information from the data. Multivariate classification methods based on machine... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_62101608" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden"> In high-energy physics, with the search for ever smaller signals in ever larger data sets, it has become essential to extract a maximum of the available information from the data. Multivariate classification methods based on machine learning techniques have ...</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/62101608" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="7dcd01bc848888f7e58938b8d1c3f83a" rel="nofollow" data-download="{"attachment_id":74955378,"asset_id":62101608,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/74955378/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="20611688" href="https://homeinteriorgallery.academia.edu/HelgeVoss">Helge Voss</a><script data-card-contents-for-user="20611688" type="text/json">{"id":20611688,"first_name":"Helge","last_name":"Voss","domain_name":"homeinteriorgallery","page_name":"HelgeVoss","display_name":"Helge Voss","profile_url":"https://homeinteriorgallery.academia.edu/HelgeVoss?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_62101608 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="62101608"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 62101608, container: ".js-paper-rank-work_62101608", }); 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$(".js-view-count[data-work-id=62101608]").text(description); $(".js-view-count-work_62101608").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_62101608").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="62101608"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">9</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="2008" href="https://www.academia.edu/Documents/in/Machine_Learning">Machine Learning</a>, <script data-card-contents-for-ri="2008" type="text/json">{"id":2008,"name":"Machine Learning","url":"https://www.academia.edu/Documents/in/Machine_Learning?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="4205" href="https://www.academia.edu/Documents/in/Data_Analysis">Data Analysis</a>, <script data-card-contents-for-ri="4205" type="text/json">{"id":4205,"name":"Data Analysis","url":"https://www.academia.edu/Documents/in/Data_Analysis?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="11119" href="https://www.academia.edu/Documents/in/User_Interface">User Interface</a>, <script data-card-contents-for-ri="11119" type="text/json">{"id":11119,"name":"User Interface","url":"https://www.academia.edu/Documents/in/User_Interface?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a><script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=62101608]'), work: {"id":62101608,"title":"TMVA-Toolkit for Multivariate Data Analysis","created_at":"2021-11-21T02:55:34.928-08:00","url":"https://www.academia.edu/62101608/TMVA_Toolkit_for_Multivariate_Data_Analysis?f_ri=14024","dom_id":"work_62101608","summary":" In high-energy physics, with the search for ever smaller signals in ever larger data sets, it has become essential to extract a maximum of the available information from the data. Multivariate classification methods based on machine learning techniques have ...","downloadable_attachments":[{"id":74955378,"asset_id":62101608,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":20611688,"first_name":"Helge","last_name":"Voss","domain_name":"homeinteriorgallery","page_name":"HelgeVoss","display_name":"Helge Voss","profile_url":"https://homeinteriorgallery.academia.edu/HelgeVoss?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":2008,"name":"Machine Learning","url":"https://www.academia.edu/Documents/in/Machine_Learning?f_ri=14024","nofollow":false},{"id":4205,"name":"Data Analysis","url":"https://www.academia.edu/Documents/in/Data_Analysis?f_ri=14024","nofollow":false},{"id":11119,"name":"User Interface","url":"https://www.academia.edu/Documents/in/User_Interface?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":23892,"name":"Multivariate Data Analysis","url":"https://www.academia.edu/Documents/in/Multivariate_Data_Analysis?f_ri=14024"},{"id":55641,"name":"Performance Evaluation","url":"https://www.academia.edu/Documents/in/Performance_Evaluation?f_ri=14024"},{"id":406250,"name":"Data Handling","url":"https://www.academia.edu/Documents/in/Data_Handling?f_ri=14024"},{"id":525017,"name":"Multivariate Regression","url":"https://www.academia.edu/Documents/in/Multivariate_Regression?f_ri=14024"},{"id":1277371,"name":"Classification Algorithm","url":"https://www.academia.edu/Documents/in/Classification_Algorithm?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_54195660" data-work_id="54195660" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/54195660/Wavelet_Analysis_of_Shower_Track_Distribution_in_High_Energy_Nucleus_Nucleus_Collisions">Wavelet Analysis of Shower Track Distribution in High-Energy Nucleus-Nucleus Collisions</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">A continuous wavelet analysis is performed for pattern recognition of charged particle emission data in28Si-Ag/Br interaction at 14.5A GeV and in32S-Ag/Br interaction at 200A GeV. Making use of the event-wise local maxima present in the... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_54195660" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">A continuous wavelet analysis is performed for pattern recognition of charged particle emission data in28Si-Ag/Br interaction at 14.5A GeV and in32S-Ag/Br interaction at 200A GeV. Making use of the event-wise local maxima present in the scalograms, we try to identify the collective behavior in multiparticle production, if there is any. For the first time, the wavelet results are compared with a model prediction based on the ultrarelativistic quantum molecular dynamics (UrQMD), where we adopt a charge reassignment algorithm to modify the UrQMD events to mimic the Bose-Einstein type of correlation among identical mesons—a feature known to be the most dominating factor responsible for local cluster formation. Statistically significant deviations between the experiment and the simulation are interpreted in terms of nontrivial dynamics of multiparticle production.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/54195660" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="3db7e046966a13aefc826dc83f5c9573" rel="nofollow" data-download="{"attachment_id":70676884,"asset_id":54195660,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/70676884/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="79968863" href="https://nbu-in.academia.edu/AmitabhaMukhopadhyay">Amitabha Mukhopadhyay</a><script data-card-contents-for-user="79968863" type="text/json">{"id":79968863,"first_name":"Amitabha","last_name":"Mukhopadhyay","domain_name":"nbu-in","page_name":"AmitabhaMukhopadhyay","display_name":"Amitabha Mukhopadhyay","profile_url":"https://nbu-in.academia.edu/AmitabhaMukhopadhyay?f_ri=14024","photo":"https://0.academia-photos.com/79968863/20597155/20208516/s65_amitabha.mukhopadhyay.jpg"}</script></span></span></li><li class="js-paper-rank-work_54195660 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="54195660"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 54195660, container: ".js-paper-rank-work_54195660", }); 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$(".js-view-count[data-work-id=54195660]").text(description); $(".js-view-count-work_54195660").attr('title', description).tooltip(); }); });</script></span><script>$(function() { $(".js-view-count-work_54195660").removeClass('hidden') })</script></div></li><li class="InlineList-item u-positionRelative" style="max-width: 250px"><div class="u-positionAbsolute" data-has-card-for-ri-list="54195660"><i class="fa fa-tag InlineList-item-icon u-positionRelative"></i>  <a class="InlineList-item-text u-positionRelative">3</a>  </div><span class="InlineList-item-text u-textTruncate u-pl9x"><a class="InlineList-item-text" data-has-card-for-ri="14024" href="https://www.academia.edu/Documents/in/High_Energy_Physics">High Energy Physics</a>, <script data-card-contents-for-ri="14024" type="text/json">{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="80414" href="https://www.academia.edu/Documents/in/Mathematical_Sciences">Mathematical Sciences</a>, <script data-card-contents-for-ri="80414" type="text/json">{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="118582" href="https://www.academia.edu/Documents/in/Physical_sciences">Physical sciences</a><script data-card-contents-for-ri="118582" type="text/json">{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=54195660]'), work: {"id":54195660,"title":"Wavelet Analysis of Shower Track Distribution in High-Energy Nucleus-Nucleus Collisions","created_at":"2021-09-30T01:09:03.332-07:00","url":"https://www.academia.edu/54195660/Wavelet_Analysis_of_Shower_Track_Distribution_in_High_Energy_Nucleus_Nucleus_Collisions?f_ri=14024","dom_id":"work_54195660","summary":"A continuous wavelet analysis is performed for pattern recognition of charged particle emission data in28Si-Ag/Br interaction at 14.5A GeV and in32S-Ag/Br interaction at 200A GeV. Making use of the event-wise local maxima present in the scalograms, we try to identify the collective behavior in multiparticle production, if there is any. For the first time, the wavelet results are compared with a model prediction based on the ultrarelativistic quantum molecular dynamics (UrQMD), where we adopt a charge reassignment algorithm to modify the UrQMD events to mimic the Bose-Einstein type of correlation among identical mesons—a feature known to be the most dominating factor responsible for local cluster formation. Statistically significant deviations between the experiment and the simulation are interpreted in terms of nontrivial dynamics of multiparticle production.","downloadable_attachments":[{"id":70676884,"asset_id":54195660,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":79968863,"first_name":"Amitabha","last_name":"Mukhopadhyay","domain_name":"nbu-in","page_name":"AmitabhaMukhopadhyay","display_name":"Amitabha Mukhopadhyay","profile_url":"https://nbu-in.academia.edu/AmitabhaMukhopadhyay?f_ri=14024","photo":"https://0.academia-photos.com/79968863/20597155/20208516/s65_amitabha.mukhopadhyay.jpg"}],"research_interests":[{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":80414,"name":"Mathematical Sciences","url":"https://www.academia.edu/Documents/in/Mathematical_Sciences?f_ri=14024","nofollow":false},{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences?f_ri=14024","nofollow":false}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_31346247" data-work_id="31346247" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/31346247/A_resolution_of_spacetime_singularity_and_black_hole_paradoxes_through_avoidance_of_trapped_surface_formation_in_Einstein_gravity">A resolution of spacetime singularity and black hole paradoxes through avoidance of trapped surface formation in Einstein gravity</a></div></div><div class="u-pb4x u-mt3x"></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue 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href="https://www.academia.edu/Documents/in/Black_Hole">Black Hole</a><script data-card-contents-for-ri="235060" type="text/json">{"id":235060,"name":"Black Hole","url":"https://www.academia.edu/Documents/in/Black_Hole?f_ri=14024","nofollow":false}</script></span></li><script>(function(){ if (true) { new Aedu.ResearchInterestListCard({ el: $('*[data-has-card-for-ri-list=31346247]'), work: {"id":31346247,"title":"A resolution of spacetime singularity and black hole paradoxes through avoidance of trapped surface formation in Einstein gravity","created_at":"2017-02-10T02:07:03.889-08:00","url":"https://www.academia.edu/31346247/A_resolution_of_spacetime_singularity_and_black_hole_paradoxes_through_avoidance_of_trapped_surface_formation_in_Einstein_gravity?f_ri=14024","dom_id":"work_31346247","summary":null,"downloadable_attachments":[{"id":51729250,"asset_id":31346247,"asset_type":"Work","always_allow_download":false}],"ordered_authors":[{"id":59856588,"first_name":"Rituparno","last_name":"Goswami","domain_name":"ukzn","page_name":"RituparnoGoswami","display_name":"Rituparno Goswami","profile_url":"https://ukzn.academia.edu/RituparnoGoswami?f_ri=14024","photo":"https://0.academia-photos.com/59856588/29986507/27842903/s65_rituparno.goswami.jpg"}],"research_interests":[{"id":6813,"name":"Quantum Cosmology","url":"https://www.academia.edu/Documents/in/Quantum_Cosmology?f_ri=14024","nofollow":false},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024","nofollow":false},{"id":128599,"name":"Gravitational Collapse","url":"https://www.academia.edu/Documents/in/Gravitational_Collapse?f_ri=14024","nofollow":false},{"id":235060,"name":"Black Hole","url":"https://www.academia.edu/Documents/in/Black_Hole?f_ri=14024","nofollow":false},{"id":679783,"name":"Boolean Satisfiability","url":"https://www.academia.edu/Documents/in/Boolean_Satisfiability?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_7137877" data-work_id="7137877" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/7137877/Quantum_criticality_and_black_holes">Quantum criticality and black holes</a></div></div><div 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href="https://www.academia.edu/Documents/in/Materials_Engineering">Materials Engineering</a>, <script data-card-contents-for-ri="56" type="text/json">{"id":56,"name":"Materials Engineering","url":"https://www.academia.edu/Documents/in/Materials_Engineering?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="505" href="https://www.academia.edu/Documents/in/Condensed_Matter_Physics">Condensed Matter Physics</a>, <script data-card-contents-for-ri="505" type="text/json">{"id":505,"name":"Condensed Matter Physics","url":"https://www.academia.edu/Documents/in/Condensed_Matter_Physics?f_ri=14024","nofollow":false}</script><a class="InlineList-item-text" data-has-card-for-ri="522" href="https://www.academia.edu/Documents/in/Thermodynamics">Thermodynamics</a>, <script data-card-contents-for-ri="522" type="text/json">{"id":522,"name":"Thermodynamics","url":"https://www.academia.edu/Documents/in/Thermodynamics?f_ri=14024","nofollow":false}</script><a 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Sachdev","profile_url":"https://harvard.academia.edu/SubirSachdev?f_ri=14024","photo":"/images/s65_no_pic.png"}],"research_interests":[{"id":56,"name":"Materials Engineering","url":"https://www.academia.edu/Documents/in/Materials_Engineering?f_ri=14024","nofollow":false},{"id":505,"name":"Condensed Matter Physics","url":"https://www.academia.edu/Documents/in/Condensed_Matter_Physics?f_ri=14024","nofollow":false},{"id":522,"name":"Thermodynamics","url":"https://www.academia.edu/Documents/in/Thermodynamics?f_ri=14024","nofollow":false},{"id":721,"name":"Magnetohydrodynamics","url":"https://www.academia.edu/Documents/in/Magnetohydrodynamics?f_ri=14024","nofollow":false},{"id":1246,"name":"Gravitation","url":"https://www.academia.edu/Documents/in/Gravitation?f_ri=14024"},{"id":2578,"name":"Particle Physics","url":"https://www.academia.edu/Documents/in/Particle_Physics?f_ri=14024"},{"id":4751,"name":"Black Holes","url":"https://www.academia.edu/Documents/in/Black_Holes?f_ri=14024"},{"id":5496,"name":"Superfluidity","url":"https://www.academia.edu/Documents/in/Superfluidity?f_ri=14024"},{"id":6469,"name":"Superconductivity","url":"https://www.academia.edu/Documents/in/Superconductivity?f_ri=14024"},{"id":10598,"name":"String Theory","url":"https://www.academia.edu/Documents/in/String_Theory?f_ri=14024"},{"id":14024,"name":"High Energy Physics","url":"https://www.academia.edu/Documents/in/High_Energy_Physics?f_ri=14024"},{"id":16460,"name":"Statistical Physics","url":"https://www.academia.edu/Documents/in/Statistical_Physics?f_ri=14024"},{"id":17733,"name":"Nanotechnology","url":"https://www.academia.edu/Documents/in/Nanotechnology?f_ri=14024"},{"id":19658,"name":"Hawking Radiation","url":"https://www.academia.edu/Documents/in/Hawking_Radiation?f_ri=14024"},{"id":34754,"name":"Magnetic field","url":"https://www.academia.edu/Documents/in/Magnetic_field?f_ri=14024"},{"id":44187,"name":"Critical phenomena","url":"https://www.academia.edu/Documents/in/Critical_phenomena?f_ri=14024"},{"id":47598,"name":"Cosmology","url":"https://www.academia.edu/Documents/in/Cosmology?f_ri=14024"},{"id":59221,"name":"Phase Diagrams","url":"https://www.academia.edu/Documents/in/Phase_Diagrams?f_ri=14024"},{"id":60653,"name":"Transport Properties","url":"https://www.academia.edu/Documents/in/Transport_Properties?f_ri=14024"},{"id":73017,"name":"Nonlinear Systems","url":"https://www.academia.edu/Documents/in/Nonlinear_Systems?f_ri=14024"},{"id":154823,"name":"Conformal Field Theory","url":"https://www.academia.edu/Documents/in/Conformal_Field_Theory?f_ri=14024"},{"id":179365,"name":"Cuprates","url":"https://www.academia.edu/Documents/in/Cuprates?f_ri=14024"},{"id":235060,"name":"Black Hole","url":"https://www.academia.edu/Documents/in/Black_Hole?f_ri=14024"},{"id":494984,"name":"Quantum Criticality","url":"https://www.academia.edu/Documents/in/Quantum_Criticality?f_ri=14024"},{"id":832541,"name":"Quantum Critical Point","url":"https://www.academia.edu/Documents/in/Quantum_Critical_Point?f_ri=14024"},{"id":936230,"name":"Quasiparticles","url":"https://www.academia.edu/Documents/in/Quasiparticles?f_ri=14024"},{"id":983074,"name":"Quantum Phase Transition","url":"https://www.academia.edu/Documents/in/Quantum_Phase_Transition?f_ri=14024"},{"id":1156863,"name":"Finite Temperature","url":"https://www.academia.edu/Documents/in/Finite_Temperature?f_ri=14024"},{"id":1483247,"name":"Kinetic Equation","url":"https://www.academia.edu/Documents/in/Kinetic_Equation?f_ri=14024"},{"id":1714286,"name":"Cuprate","url":"https://www.academia.edu/Documents/in/Cuprate?f_ri=14024"}]}, }) } })();</script></ul></li></ul></div></div><div class="u-borderBottom1 u-borderColorGrayLighter"><div class="clearfix u-pv7x u-mb0x js-work-card work_27297223" data-work_id="27297223" itemscope="itemscope" itemtype="https://schema.org/ScholarlyArticle"><div class="header"><div class="title u-fontSerif u-fs22 u-lineHeight1_3"><a class="u-tcGrayDarkest js-work-link" href="https://www.academia.edu/27297223/Dissipative_superfluids_from_cold_atoms_to_quark_matter">Dissipative superfluids, from cold atoms to quark matter</a></div></div><div class="u-pb4x u-mt3x"><div class="summary u-fs14 u-fw300 u-lineHeight1_5 u-tcGrayDarkest"><div class="summarized">Some results about dissipative processes in superfluids are presented. We focus on fermionic superfluidity and restrict our analysis to the contribution of phonons to bulk viscosity, shear viscosity and thermal conductivity. At... <a class="more_link u-tcGrayDark u-linkUnstyled" data-container=".work_27297223" data-show=".complete" data-hide=".summarized" data-more-link-behavior="true" href="#">more</a></div><div class="complete hidden">Some results about dissipative processes in superfluids are presented. We focus on fermionic superfluidity and restrict our analysis to the contribution of phonons to bulk viscosity, shear viscosity and thermal conductivity. At sufficiently low temperatures phonons give the dominant contribution to the transport coefficients if all the other low energy excitation of the system are gapped. We first consider a system of cold fermionic atoms close to the unitarity limit. Then we turn to the superfluid phase of quark matter that may be realized at high baryonic density.</div></div></div><ul class="InlineList u-ph0x u-fs13"><li class="InlineList-item logged_in_only"><div class="share_on_academia_work_button"><a class="academia_share Button Button--inverseBlue Button--sm js-bookmark-button" data-academia-share="Work/27297223" data-share-source="work_strip" data-spinner="small_white_hide_contents"><i class="fa fa-plus"></i><span class="work-strip-link-text u-ml1x" data-content="button_text">Bookmark</span></a></div></li><li class="InlineList-item"><div class="download"><a id="ddb8b39393fb89503fda7cd12443411a" rel="nofollow" data-download="{"attachment_id":47555477,"asset_id":27297223,"asset_type":"Work","always_allow_download":false,"track":null,"button_location":"work_strip","source":null,"hide_modal":null}" class="Button Button--sm Button--inverseGreen js-download-button prompt_button doc_download" href="https://www.academia.edu/attachments/47555477/download_file?st=MTczMjQyMzQ5OCw4LjIyMi4yMDguMTQ2&s=work_strip"><i class="fa fa-arrow-circle-o-down fa-lg"></i><span class="u-textUppercase u-ml1x" data-content="button_text">Download</span></a></div></li><li class="InlineList-item"><ul class="InlineList InlineList--bordered u-ph0x"><li class="InlineList-item InlineList-item--bordered"><span class="InlineList-item-text">by <span itemscope="itemscope" itemprop="author" itemtype="https://schema.org/Person"><a class="u-tcGrayDark u-fw700" data-has-card-for-user="51363599" href="https://independent.academia.edu/CristinaManuel1">Cristina Manuel</a><script data-card-contents-for-user="51363599" type="text/json">{"id":51363599,"first_name":"Cristina","last_name":"Manuel","domain_name":"independent","page_name":"CristinaManuel1","display_name":"Cristina Manuel","profile_url":"https://independent.academia.edu/CristinaManuel1?f_ri=14024","photo":"/images/s65_no_pic.png"}</script></span></span></li><li class="js-paper-rank-work_27297223 InlineList-item InlineList-item--bordered hidden"><span class="js-paper-rank-view hidden u-tcGrayDark" data-paper-rank-work-id="27297223"><i class="u-m1x fa fa-bar-chart"></i><strong class="js-paper-rank"></strong></span><script>$(function() { new Works.PaperRankView({ workId: 27297223, container: ".js-paper-rank-work_27297223", }); 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