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class="js-profile-view-count"></span></p></div></span></div><div class="ri-section"><div class="ri-section-header"><span>Interests</span></div><div class="ri-tags-container"><a data-click-track="profile-user-info-expand-research-interests" data-has-card-for-ri-list="47139266" href="https://www.academia.edu/Documents/in/Loop_Quantum_Gravity"><div id="js-react-on-rails-context" style="display:none" data-rails-context="{"inMailer":false,"i18nLocale":"en","i18nDefaultLocale":"en","href":"https://independent.academia.edu/RomeshKaul","location":"/RomeshKaul","scheme":"https","host":"independent.academia.edu","port":null,"pathname":"/RomeshKaul","search":null,"httpAcceptLanguage":null,"serverSide":false}"></div> <div class="js-react-on-rails-component" style="display:none" data-component-name="Pill" data-props="{"color":"gray","children":["Loop Quantum Gravity"]}" data-trace="false" data-dom-id="Pill-react-component-67789e4e-1f29-48ca-8745-c8a5d5f0be82"></div> <div id="Pill-react-component-67789e4e-1f29-48ca-8745-c8a5d5f0be82"></div> </a><a data-click-track="profile-user-info-expand-research-interests" data-has-card-for-ri-list="47139266" href="https://www.academia.edu/Documents/in/Field_Theory"><div class="js-react-on-rails-component" style="display:none" data-component-name="Pill" data-props="{"color":"gray","children":["Field Theory"]}" data-trace="false" data-dom-id="Pill-react-component-73d7051c-75b1-4f30-90c4-c059f1d8f2db"></div> <div id="Pill-react-component-73d7051c-75b1-4f30-90c4-c059f1d8f2db"></div> </a><a data-click-track="profile-user-info-expand-research-interests" data-has-card-for-ri-list="47139266" href="https://www.academia.edu/Documents/in/Pure_Mathematics"><div class="js-react-on-rails-component" style="display:none" data-component-name="Pill" data-props="{"color":"gray","children":["Pure Mathematics"]}" data-trace="false" data-dom-id="Pill-react-component-3f604f07-7e0b-4626-974e-5c01de82bfd5"></div> <div 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id="Pill-react-component-b944236b-c3d0-4f1a-a33d-a97e3abc3e9b"></div> </a></div></div></div></div><div class="right-panel-container"><div class="user-content-wrapper"><div class="uploads-container" id="social-redesign-work-container"><div class="upload-header"><h2 class="ds2-5-heading-sans-serif-xs">Uploads</h2></div><div class="documents-container backbone-social-profile-documents" style="width: 100%;"><div class="u-taCenter"></div><div class="profile--tab_content_container js-tab-pane tab-pane active" id="all"><div class="profile--tab_heading_container js-section-heading" data-section="Papers" id="Papers"><h3 class="profile--tab_heading_container">Papers by Romesh Kaul</h3></div><div class="js-work-strip profile--work_container" data-work-id="24498112"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498112/Supersymmetric_solution_of_gauge_hierarchy_problem"><img alt="Research paper thumbnail of Supersymmetric solution of gauge hierarchy problem" class="work-thumbnail" src="https://a.academia-assets.com/images/blank-paper.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498112/Supersymmetric_solution_of_gauge_hierarchy_problem">Supersymmetric solution of gauge hierarchy problem</a></div><div class="wp-workCard_item"><span>Pramana</span><span>, 1982</span></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Some recent developments with respect to the resolution of the gauge hierarchy problem in grand u...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Some recent developments with respect to the resolution of the gauge hierarchy problem in grand unified theories by supersymmetry are presented. A general argument is developed to show how global supersymmetry maintains the stability of the different mass-scales under perturbative effects.</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498112"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498112"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498112; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498112]").text(description); $(".js-view-count[data-work-id=24498112]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498112; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498112']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498112, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498112]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498112,"title":"Supersymmetric solution of gauge hierarchy problem","translated_title":"","metadata":{"abstract":"Some recent developments with respect to the resolution of the gauge hierarchy problem in grand unified theories by supersymmetry are presented. 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498108"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" rel="nofollow" href="https://www.academia.edu/24498108/Degenerate_spacetimes_in_first_order_gravity"><img alt="Research paper thumbnail of Degenerate spacetimes in first order gravity" class="work-thumbnail" src="https://a.academia-assets.com/images/blank-paper.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" rel="nofollow" href="https://www.academia.edu/24498108/Degenerate_spacetimes_in_first_order_gravity">Degenerate spacetimes in first order gravity</a></div><div class="wp-workCard_item"><span>Physical Review D</span><span>, 2016</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498108"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498108"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498108; 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498106"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498106/Topological_parameters_in_gravity"><img alt="Research paper thumbnail of Topological parameters in gravity" class="work-thumbnail" src="https://attachments.academia-assets.com/44830214/thumbnails/1.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498106/Topological_parameters_in_gravity">Topological parameters in gravity</a></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">We present the Hamiltonian analysis of the theory of gravity based on a Lagrangian density contai...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">We present the Hamiltonian analysis of the theory of gravity based on a Lagrangian density containing Hilbert-Palatini term along with three topological densities, Nieh-Yan, Pontryagin and Euler. The addition of these topological terms modifies the symplectic structure non-trivially. The resulting canonical theory develops a dependence on three parameters which are coefficients of these terms. 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While quantum field the...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">The Principle of Naturalness of small parameters of a theory is reviewed. While quantum field theories constructed from gauge fields and fermions only are natural, those containing elementary scalar fields are not. In particular the Higgs boson mass in the Standard Model of electro-weak forces is not stable against radiative corrections. Two old canonical solutions of this problem are: (i)</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="7bead24f5d8b7cd9fa637c2f8af45068" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830213,"asset_id":24498105,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830213/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498105"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498105"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498105; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498105]").text(description); $(".js-view-count[data-work-id=24498105]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498105; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498105']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498105, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "7bead24f5d8b7cd9fa637c2f8af45068" } } $('.js-work-strip[data-work-id=24498105]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498105,"title":"Naturalness and Electroweak Symmetry Breaking","translated_title":"","metadata":{"abstract":"The Principle of Naturalness of small parameters of a theory is reviewed. 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498104"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498104/Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants"><img alt="Research paper thumbnail of Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants" class="work-thumbnail" src="https://attachments.academia-assets.com/44830217/thumbnails/1.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498104/Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants">Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants</a></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Chern-Simons theories, which are topological quantum field theories, provide a field theoretic fr...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Chern-Simons theories, which are topological quantum field theories, provide a field theoretic framework for the study of knots and links in three dimensions. These are rare examples of quantum field theories which can be exactly and explicitly solved. Expectation values of Wilson link operators yield a class of link invariants, the simplest of them is the famous Jones polynomial. Other</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="5916d995d939f6010c0cb997ec001502" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830217,"asset_id":24498104,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830217/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498104"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498104"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498104; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498104]").text(description); $(".js-view-count[data-work-id=24498104]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498104; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498104']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498104, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "5916d995d939f6010c0cb997ec001502" } } $('.js-work-strip[data-work-id=24498104]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498104,"title":"Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants","translated_title":"","metadata":{"abstract":"Chern-Simons theories, which are topological quantum field theories, provide a field theoretic framework for the study of knots and links in three dimensions. 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Other","internal_url":"https://www.academia.edu/24498104/Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants","translated_internal_url":"","created_at":"2016-04-17T13:54:09.268-07:00","preview_url":null,"current_user_can_edit":null,"current_user_is_owner":null,"owner_id":47139266,"coauthors_can_edit":true,"document_type":"paper","co_author_tags":[],"downloadable_attachments":[{"id":44830217,"title":"","file_type":"pdf","scribd_thumbnail_url":"https://attachments.academia-assets.com/44830217/thumbnails/1.jpg","file_name":"9804122.pdf","download_url":"https://www.academia.edu/attachments/44830217/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&","bulk_download_file_name":"Chern_Simons_Theory_Knot_Invariants_Vert.pdf","bulk_download_url":"https://d1wqtxts1xzle7.cloudfront.net/44830217/9804122-libre.pdf?1460926517=\u0026response-content-disposition=attachment%3B+filename%3DChern_Simons_Theory_Knot_Invariants_Vert.pdf\u0026Expires=1732435402\u0026Signature=RKjYCuSTRxh9XlJC6HMxxAoLI5mYCFJQXVGXUxz9v1hJeMgIaRNV-xFB3AyprPVjpYUaW1wZA93~sJ7Ao-G0OG3qlZmX~kra7AqJpHXAD~vDFcWcdE61Z0VxrZf3UN6nvw0-zgCD-x--jlnVpKT2gZMmAM227ZWwrVj93TofsNKnR~0dTMuwEg0Peqp~h1GyIT5D-IRumyvUWK4gTNIfNT9-8zJhP5w7gn7RxKs-lKN95CDWW8dYtIXdjdA515Tld0EDvjiTtQR6wSsGTwP~edlbb7wU1CnYcEGGV6Cap~fQLGWMZT8t5XyZj~1lXG4kEBSJwKA0pwEegpvWdRhFjA__\u0026Key-Pair-Id=APKAJLOHF5GGSLRBV4ZA"}],"slug":"Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants","translated_slug":"","page_count":27,"language":"en","content_type":"Work","owner":{"id":47139266,"first_name":"Romesh","middle_initials":null,"last_name":"Kaul","page_name":"RomeshKaul","domain_name":"independent","created_at":"2016-04-16T02:35:37.265-07:00","display_name":"Romesh Kaul","url":"https://independent.academia.edu/RomeshKaul"},"attachments":[{"id":44830217,"title":"","file_type":"pdf","scribd_thumbnail_url":"https://attachments.academia-assets.com/44830217/thumbnails/1.jpg","file_name":"9804122.pdf","download_url":"https://www.academia.edu/attachments/44830217/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&","bulk_download_file_name":"Chern_Simons_Theory_Knot_Invariants_Vert.pdf","bulk_download_url":"https://d1wqtxts1xzle7.cloudfront.net/44830217/9804122-libre.pdf?1460926517=\u0026response-content-disposition=attachment%3B+filename%3DChern_Simons_Theory_Knot_Invariants_Vert.pdf\u0026Expires=1732435402\u0026Signature=RKjYCuSTRxh9XlJC6HMxxAoLI5mYCFJQXVGXUxz9v1hJeMgIaRNV-xFB3AyprPVjpYUaW1wZA93~sJ7Ao-G0OG3qlZmX~kra7AqJpHXAD~vDFcWcdE61Z0VxrZf3UN6nvw0-zgCD-x--jlnVpKT2gZMmAM227ZWwrVj93TofsNKnR~0dTMuwEg0Peqp~h1GyIT5D-IRumyvUWK4gTNIfNT9-8zJhP5w7gn7RxKs-lKN95CDWW8dYtIXdjdA515Tld0EDvjiTtQR6wSsGTwP~edlbb7wU1CnYcEGGV6Cap~fQLGWMZT8t5XyZj~1lXG4kEBSJwKA0pwEegpvWdRhFjA__\u0026Key-Pair-Id=APKAJLOHF5GGSLRBV4ZA"},{"id":44830216,"title":"","file_type":"pdf","scribd_thumbnail_url":"https://attachments.academia-assets.com/44830216/thumbnails/1.jpg","file_name":"9804122.pdf","download_url":"https://www.academia.edu/attachments/44830216/download_file","bulk_download_file_name":"Chern_Simons_Theory_Knot_Invariants_Vert.pdf","bulk_download_url":"https://d1wqtxts1xzle7.cloudfront.net/44830216/9804122-libre.pdf?1460926518=\u0026response-content-disposition=attachment%3B+filename%3DChern_Simons_Theory_Knot_Invariants_Vert.pdf\u0026Expires=1732435402\u0026Signature=EFiBOpiGF2BolQ7DXhNbBoB4byhhosqA83l2o474K3FKuL-qfL26Jyi90Z~dWKVhse5yfnMYVAOfrv1xYWVhY~MgEIGjV~dT0vxi55cpkTgn0WzT7C906316fmAspo9mAwRh5nWqb1Q1dro~TNMedSUqcN8nSgb2VTuOqz~hntJ2C-aZHouh~zo5grVqZgjHi-6fWgFG2dErpilDA33nvdTO7hksevu4X8EgZSwZcgF-VaofxT2g-x4okEwLTW7i0dhNkYBmcCegHqGy9Ww~yR7bMM4UWVi5AKme4N5p0Qdx55R-1BGZoChNXlrgPFhKgFAFzmRxVDkHXVbL2KPvkg__\u0026Key-Pair-Id=APKAJLOHF5GGSLRBV4ZA"}],"research_interests":[{"id":4427,"name":"Topological Quantum Field Theory","url":"https://www.academia.edu/Documents/in/Topological_Quantum_Field_Theory"},{"id":10092,"name":"Quantum Field Theory","url":"https://www.academia.edu/Documents/in/Quantum_Field_Theory"},{"id":364279,"name":"Chern Simons Theory","url":"https://www.academia.edu/Documents/in/Chern_Simons_Theory"},{"id":412636,"name":"Theoretical Framework","url":"https://www.academia.edu/Documents/in/Theoretical_Framework"},{"id":1296393,"name":"Crossing Number","url":"https://www.academia.edu/Documents/in/Crossing_Number"}],"urls":[{"id":7024528,"url":"http://arxiv.org/abs/hep-th/9804122"}]}, dispatcherData: dispatcherData }); $(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498103"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498103/The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model"><img alt="Research paper thumbnail of The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model" class="work-thumbnail" src="https://a.academia-assets.com/images/blank-paper.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498103/The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model">The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model</a></div><div class="wp-workCard_item"><span>Physics Letters B</span><span>, 1983</span></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Using the dimensional reduction regularization scheme, we show that radiative corrections to the ...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Using the dimensional reduction regularization scheme, we show that radiative corrections to the anomaly of the axial current, which is coupled to the gauge field, are absent in a supersymmetric U(1) gauge model for both &amp;#39;t Hooft-Veltman and Bardeen prescriptions for gamma5. We also discuss the results with reference to conventional dimensional regularization. This result has significant implications with respect</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498103"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498103"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498103; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498103]").text(description); $(".js-view-count[data-work-id=24498103]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498103; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498103']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498103, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498103]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498103,"title":"The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model","translated_title":"","metadata":{"abstract":"Using the dimensional reduction regularization scheme, we show that radiative corrections to the anomaly of the axial current, which is coupled to the gauge field, are absent in a supersymmetric U(1) gauge model for both \u0026amp;#39;t Hooft-Veltman and Bardeen prescriptions for gamma5. 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To this effect the necessary aspects of the theory of coloured-oriented braids and duality properties of conformal blocks for the correlators of SU(2) k Wess-Zumino conformal field theory are presented. A large class of representations of the generators of the groupoid of coloured-oriented braids are obtained. These provide a whole lot of new link invariants of which Jones polynomials are the simplest examples. These new invariants are explicity calculated as illustrations for knots up to eight crossings and twocomponent multicoloured links up to seven crossings.</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="d5fb637f1495d1812e3c885fc3845613" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830250,"asset_id":24498102,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830250/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498102"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498102"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498102; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498102]").text(description); $(".js-view-count[data-work-id=24498102]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498102; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498102']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498102, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "d5fb637f1495d1812e3c885fc3845613" } } $('.js-work-strip[data-work-id=24498102]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498102,"title":"Chern-Simons theory, coloured-oriented braids and link invariants","translated_title":"","metadata":{"abstract":"A method to obtain explicit and complete topological solution of SU(2) Chern-Simons theory on S 3 is developed. 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To this effect the necessary aspects of the theory of coloured-oriented braids and duality properties of conformal blocks for the correlators of SU(2) k Wess-Zumino conformal field theory are presented. A large class of representations of the generators of the groupoid of coloured-oriented braids are obtained. These provide a whole lot of new link invariants of which Jones polynomials are the simplest examples. 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498090"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498090/Entropy_of_Quantum_Black_Holes"><img alt="Research paper thumbnail of Entropy of Quantum Black Holes" class="work-thumbnail" src="https://attachments.academia-assets.com/44830242/thumbnails/1.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498090/Entropy_of_Quantum_Black_Holes">Entropy of Quantum Black Holes</a></div><div class="wp-workCard_item"><span>Symmetry, Integrability and Geometry: Methods and Applications</span><span>, 2012</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="baf8cf0ddc2d17183d610640ca800d79" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830242,"asset_id":24498090,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830242/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498090"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498090"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498090; 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There is an equivalent formulation of the horizon degrees of freedom in terms of a U (1) gauge theory which is just a gauged fixed version of the SU (2) theory. These developments will be surveyed here. Quantum theory based on either formulation can be used to count the horizon micro-states associated with quantum geometry fluctuations and from this the micro-canonical entropy can be obtained. We shall review the computation in SU (2) formulation. Leading term in the entropy is proportional to horizon area with a coefficient depending on the Barbero-Immirzi parameter which is fixed by matching this result with the Bekenstein-Hawking formula. Remarkably there are corrections beyond the area term, the leading one is logarithm of the horizon area with a definite coefficient −3/2, a result which is more than a decade old now. How the same results are obtained in the equivalent U (1) framework will also be indicated. Over years, this entropy formula has also been arrived at from a variety of other perspectives. In particular, entropy of BTZ black holes in three dimensional gravity exhibits the same logarithmic correction. Even in the String Theory, many black hole models are known to possess such properties. 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It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. There are two solutions to this problem: (i) a global supersymmetry, which ensures the absence of all</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498089"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498089"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498089; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498089]").text(description); $(".js-view-count[data-work-id=24498089]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498089; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498089']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498089, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498089]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498089,"title":"Technicolor","translated_title":"","metadata":{"abstract":"The need for reexamination of the standard model of strong, weak, and electromagnetic interactions is discussed, especially with regard to \u0026amp;#39;t Hooft\u0026amp;#39;s criterion of naturalness. It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. There are two solutions to this problem: (i) a global supersymmetry, which ensures the absence of all","publication_date":{"day":null,"month":null,"year":1983,"errors":{}},"publication_name":"Reviews of Modern Physics"},"translated_abstract":"The need for reexamination of the standard model of strong, weak, and electromagnetic interactions is discussed, especially with regard to \u0026amp;#39;t Hooft\u0026amp;#39;s criterion of naturalness. It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. There are two solutions to this problem: (i) a global supersymmetry, which ensures the absence of all","internal_url":"https://www.academia.edu/24498089/Technicolor","translated_internal_url":"","created_at":"2016-04-17T13:54:06.117-07:00","preview_url":null,"current_user_can_edit":null,"current_user_is_owner":null,"owner_id":47139266,"coauthors_can_edit":true,"document_type":"paper","co_author_tags":[],"downloadable_attachments":[],"slug":"Technicolor","translated_slug":"","page_count":null,"language":"en","content_type":"Work","owner":{"id":47139266,"first_name":"Romesh","middle_initials":null,"last_name":"Kaul","page_name":"RomeshKaul","domain_name":"independent","created_at":"2016-04-16T02:35:37.265-07:00","display_name":"Romesh Kaul","url":"https://independent.academia.edu/RomeshKaul"},"attachments":[],"research_interests":[{"id":118582,"name":"Physical sciences","url":"https://www.academia.edu/Documents/in/Physical_sciences"}],"urls":[]}, dispatcherData: dispatcherData }); $(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> </div><div class="profile--tab_content_container js-tab-pane tab-pane" data-section-id="5047913" id="papers"><div class="js-work-strip profile--work_container" data-work-id="24498112"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498112/Supersymmetric_solution_of_gauge_hierarchy_problem"><img alt="Research paper thumbnail of Supersymmetric solution of gauge hierarchy problem" class="work-thumbnail" src="https://a.academia-assets.com/images/blank-paper.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498112/Supersymmetric_solution_of_gauge_hierarchy_problem">Supersymmetric solution of gauge hierarchy problem</a></div><div class="wp-workCard_item"><span>Pramana</span><span>, 1982</span></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Some recent developments with respect to the resolution of the gauge hierarchy problem in grand u...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Some recent developments with respect to the resolution of the gauge hierarchy problem in grand unified theories by supersymmetry are presented. A general argument is developed to show how global supersymmetry maintains the stability of the different mass-scales under perturbative effects.</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498112"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498112"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498112; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498112]").text(description); $(".js-view-count[data-work-id=24498112]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498112; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498112']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498112, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498112]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498112,"title":"Supersymmetric solution of gauge hierarchy problem","translated_title":"","metadata":{"abstract":"Some recent developments with respect to the resolution of the gauge hierarchy problem in grand unified theories by supersymmetry are presented. 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The addition of these topological terms modifies the symplectic structure non-trivially. The resulting canonical theory develops a dependence on three parameters which are coefficients of these terms. In the time gauge, we obtain</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="a4b7946bc4394bff787001b55afc2293" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830214,"asset_id":24498106,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830214/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498106"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498106"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498106; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498106]").text(description); $(".js-view-count[data-work-id=24498106]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498106; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498106']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498106, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "a4b7946bc4394bff787001b55afc2293" } } $('.js-work-strip[data-work-id=24498106]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498106,"title":"Topological parameters in gravity","translated_title":"","metadata":{"abstract":"We present the Hamiltonian analysis of the theory of gravity based on a Lagrangian density containing Hilbert-Palatini term along with three topological densities, Nieh-Yan, Pontryagin and Euler. 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While quantum field the...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">The Principle of Naturalness of small parameters of a theory is reviewed. While quantum field theories constructed from gauge fields and fermions only are natural, those containing elementary scalar fields are not. In particular the Higgs boson mass in the Standard Model of electro-weak forces is not stable against radiative corrections. Two old canonical solutions of this problem are: (i)</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="7bead24f5d8b7cd9fa637c2f8af45068" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830213,"asset_id":24498105,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830213/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498105"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498105"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498105; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498105]").text(description); $(".js-view-count[data-work-id=24498105]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498105; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498105']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498105, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "7bead24f5d8b7cd9fa637c2f8af45068" } } $('.js-work-strip[data-work-id=24498105]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498105,"title":"Naturalness and Electroweak Symmetry Breaking","translated_title":"","metadata":{"abstract":"The Principle of Naturalness of small parameters of a theory is reviewed. 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498104"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498104/Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants"><img alt="Research paper thumbnail of Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants" class="work-thumbnail" src="https://attachments.academia-assets.com/44830217/thumbnails/1.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498104/Chern_Simons_Theory_Knot_Invariants_Vertex_Models_and_Three_manifold_Invariants">Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants</a></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Chern-Simons theories, which are topological quantum field theories, provide a field theoretic fr...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Chern-Simons theories, which are topological quantum field theories, provide a field theoretic framework for the study of knots and links in three dimensions. These are rare examples of quantum field theories which can be exactly and explicitly solved. Expectation values of Wilson link operators yield a class of link invariants, the simplest of them is the famous Jones polynomial. Other</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="5916d995d939f6010c0cb997ec001502" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830217,"asset_id":24498104,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830217/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498104"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498104"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498104; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498104]").text(description); $(".js-view-count[data-work-id=24498104]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498104; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498104']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498104, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "5916d995d939f6010c0cb997ec001502" } } $('.js-work-strip[data-work-id=24498104]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498104,"title":"Chern-Simons Theory, Knot Invariants, Vertex Models and Three-manifold Invariants","translated_title":"","metadata":{"abstract":"Chern-Simons theories, which are topological quantum field theories, provide a field theoretic framework for the study of knots and links in three dimensions. 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$(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498103"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498103/The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model"><img alt="Research paper thumbnail of The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model" class="work-thumbnail" src="https://a.academia-assets.com/images/blank-paper.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498103/The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model">The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model</a></div><div class="wp-workCard_item"><span>Physics Letters B</span><span>, 1983</span></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">Using the dimensional reduction regularization scheme, we show that radiative corrections to the ...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">Using the dimensional reduction regularization scheme, we show that radiative corrections to the anomaly of the axial current, which is coupled to the gauge field, are absent in a supersymmetric U(1) gauge model for both &amp;#39;t Hooft-Veltman and Bardeen prescriptions for gamma5. We also discuss the results with reference to conventional dimensional regularization. This result has significant implications with respect</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498103"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498103"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498103; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498103]").text(description); $(".js-view-count[data-work-id=24498103]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498103; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498103']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498103, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498103]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498103,"title":"The validity of the Adler-Bardeen theorem in the supersymmetric U(1) gauge model","translated_title":"","metadata":{"abstract":"Using the dimensional reduction regularization scheme, we show that radiative corrections to the anomaly of the axial current, which is coupled to the gauge field, are absent in a supersymmetric U(1) gauge model for both \u0026amp;#39;t Hooft-Veltman and Bardeen prescriptions for gamma5. We also discuss the results with reference to conventional dimensional regularization. This result has significant implications with respect","publication_date":{"day":null,"month":null,"year":1983,"errors":{}},"publication_name":"Physics Letters B"},"translated_abstract":"Using the dimensional reduction regularization scheme, we show that radiative corrections to the anomaly of the axial current, which is coupled to the gauge field, are absent in a supersymmetric U(1) gauge model for both \u0026amp;#39;t Hooft-Veltman and Bardeen prescriptions for gamma5. We also discuss the results with reference to conventional dimensional regularization. This result has significant implications with respect","internal_url":"https://www.academia.edu/24498103/The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model","translated_internal_url":"","created_at":"2016-04-17T13:54:09.022-07:00","preview_url":null,"current_user_can_edit":null,"current_user_is_owner":null,"owner_id":47139266,"coauthors_can_edit":true,"document_type":"paper","co_author_tags":[],"downloadable_attachments":[],"slug":"The_validity_of_the_Adler_Bardeen_theorem_in_the_supersymmetric_U_1_gauge_model","translated_slug":"","page_count":null,"language":"en","content_type":"Work","owner":{"id":47139266,"first_name":"Romesh","middle_initials":null,"last_name":"Kaul","page_name":"RomeshKaul","domain_name":"independent","created_at":"2016-04-16T02:35:37.265-07:00","display_name":"Romesh Kaul","url":"https://independent.academia.edu/RomeshKaul"},"attachments":[],"research_interests":[{"id":27762,"name":"Supersymmetric Models","url":"https://www.academia.edu/Documents/in/Supersymmetric_Models"},{"id":403158,"name":"Gauge Field","url":"https://www.academia.edu/Documents/in/Gauge_Field"}],"urls":[]}, dispatcherData: dispatcherData }); $(this).data('initialized', true); } }); $a.trackClickSource(".js-work-strip-work-link", "profile_work_strip") }); </script> <div class="js-work-strip profile--work_container" data-work-id="24498102"><div class="profile--work_thumbnail hidden-xs"><a class="js-work-strip-work-link" data-click-track="profile-work-strip-thumbnail" href="https://www.academia.edu/24498102/Chern_Simons_theory_coloured_oriented_braids_and_link_invariants"><img alt="Research paper thumbnail of Chern-Simons theory, coloured-oriented braids and link invariants" class="work-thumbnail" src="https://attachments.academia-assets.com/44830250/thumbnails/1.jpg" /></a></div><div class="wp-workCard wp-workCard_itemContainer"><div class="wp-workCard_item wp-workCard--title"><a class="js-work-strip-work-link text-gray-darker" data-click-track="profile-work-strip-title" href="https://www.academia.edu/24498102/Chern_Simons_theory_coloured_oriented_braids_and_link_invariants">Chern-Simons theory, coloured-oriented braids and link invariants</a></div><div class="wp-workCard_item"><span>Communications in Mathematical Physics</span><span>, 1994</span></div><div class="wp-workCard_item"><span class="js-work-more-abstract-truncated">A method to obtain explicit and complete topological solution of SU(2) Chern-Simons theory on S 3...</span><a class="js-work-more-abstract" data-broccoli-component="work_strip.more_abstract" data-click-track="profile-work-strip-more-abstract" href="javascript:;"><span> more </span><span><i class="fa fa-caret-down"></i></span></a><span class="js-work-more-abstract-untruncated hidden">A method to obtain explicit and complete topological solution of SU(2) Chern-Simons theory on S 3 is developed. To this effect the necessary aspects of the theory of coloured-oriented braids and duality properties of conformal blocks for the correlators of SU(2) k Wess-Zumino conformal field theory are presented. A large class of representations of the generators of the groupoid of coloured-oriented braids are obtained. These provide a whole lot of new link invariants of which Jones polynomials are the simplest examples. These new invariants are explicity calculated as illustrations for knots up to eight crossings and twocomponent multicoloured links up to seven crossings.</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><a id="d5fb637f1495d1812e3c885fc3845613" class="wp-workCard--action" rel="nofollow" data-click-track="profile-work-strip-download" data-download="{"attachment_id":44830250,"asset_id":24498102,"asset_type":"Work","button_location":"profile"}" href="https://www.academia.edu/attachments/44830250/download_file?st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&st=MTczMjQzMTgwMiw4LjIyMi4yMDguMTQ2&s=profile"><span><i class="fa fa-arrow-down"></i></span><span>Download</span></a><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498102"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498102"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498102; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498102]").text(description); $(".js-view-count[data-work-id=24498102]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498102; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498102']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498102, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (true){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "d5fb637f1495d1812e3c885fc3845613" } } $('.js-work-strip[data-work-id=24498102]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498102,"title":"Chern-Simons theory, coloured-oriented braids and link invariants","translated_title":"","metadata":{"abstract":"A method to obtain explicit and complete topological solution of SU(2) Chern-Simons theory on S 3 is developed. To this effect the necessary aspects of the theory of coloured-oriented braids and duality properties of conformal blocks for the correlators of SU(2) k Wess-Zumino conformal field theory are presented. A large class of representations of the generators of the groupoid of coloured-oriented braids are obtained. These provide a whole lot of new link invariants of which Jones polynomials are the simplest examples. These new invariants are explicity calculated as illustrations for knots up to eight crossings and twocomponent multicoloured links up to seven crossings.","publication_date":{"day":null,"month":null,"year":1994,"errors":{}},"publication_name":"Communications in Mathematical Physics"},"translated_abstract":"A method to obtain explicit and complete topological solution of SU(2) Chern-Simons theory on S 3 is developed. 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There is an equivalent formulation of the horizon degrees of freedom in terms of a U (1) gauge theory which is just a gauged fixed version of the SU (2) theory. These developments will be surveyed here. Quantum theory based on either formulation can be used to count the horizon micro-states associated with quantum geometry fluctuations and from this the micro-canonical entropy can be obtained. We shall review the computation in SU (2) formulation. Leading term in the entropy is proportional to horizon area with a coefficient depending on the Barbero-Immirzi parameter which is fixed by matching this result with the Bekenstein-Hawking formula. Remarkably there are corrections beyond the area term, the leading one is logarithm of the horizon area with a definite coefficient −3/2, a result which is more than a decade old now. How the same results are obtained in the equivalent U (1) framework will also be indicated. Over years, this entropy formula has also been arrived at from a variety of other perspectives. In particular, entropy of BTZ black holes in three dimensional gravity exhibits the same logarithmic correction. Even in the String Theory, many black hole models are known to possess such properties. 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It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. There are two solutions to this problem: (i) a global supersymmetry, which ensures the absence of all</span></div><div class="wp-workCard_item wp-workCard--actions"><span class="work-strip-bookmark-button-container"></span><span class="wp-workCard--action visible-if-viewed-by-owner inline-block" style="display: none;"><span class="js-profile-work-strip-edit-button-wrapper profile-work-strip-edit-button-wrapper" data-work-id="24498089"><a class="js-profile-work-strip-edit-button" tabindex="0"><span><i class="fa fa-pencil"></i></span><span>Edit</span></a></span></span><span id="work-strip-rankings-button-container"></span></div><div class="wp-workCard_item wp-workCard--stats"><span><span><span class="js-view-count view-count u-mr2x" data-work-id="24498089"><i class="fa fa-spinner fa-spin"></i></span><script>$(function () { var workId = 24498089; window.Academia.workViewCountsFetcher.queue(workId, function (count) { var description = window.$h.commaizeInt(count) + " " + window.$h.pluralize(count, 'View'); $(".js-view-count[data-work-id=24498089]").text(description); $(".js-view-count[data-work-id=24498089]").attr('title', description).tooltip(); }); });</script></span></span><span><span class="percentile-widget hidden"><span class="u-mr2x work-percentile"></span></span><script>$(function () { var workId = 24498089; window.Academia.workPercentilesFetcher.queue(workId, function (percentileText) { var container = $(".js-work-strip[data-work-id='24498089']"); container.find('.work-percentile').text(percentileText.charAt(0).toUpperCase() + percentileText.slice(1)); container.find('.percentile-widget').show(); container.find('.percentile-widget').removeClass('hidden'); }); });</script></span><span><script>$(function() { new Works.PaperRankView({ workId: 24498089, container: "", }); });</script></span></div><div id="work-strip-premium-row-container"></div></div></div><script> require.config({ waitSeconds: 90 })(["https://a.academia-assets.com/assets/wow_profile-f77ea15d77ce96025a6048a514272ad8becbad23c641fc2b3bd6e24ca6ff1932.js","https://a.academia-assets.com/assets/work_edit-ad038b8c047c1a8d4fa01b402d530ff93c45fee2137a149a4a5398bc8ad67560.js"], function() { // from javascript_helper.rb var dispatcherData = {} if (false){ window.WowProfile.dispatcher = window.WowProfile.dispatcher || _.clone(Backbone.Events); dispatcherData = { dispatcher: window.WowProfile.dispatcher, downloadLinkId: "-1" } } $('.js-work-strip[data-work-id=24498089]').each(function() { if (!$(this).data('initialized')) { new WowProfile.WorkStripView({ el: this, workJSON: {"id":24498089,"title":"Technicolor","translated_title":"","metadata":{"abstract":"The need for reexamination of the standard model of strong, weak, and electromagnetic interactions is discussed, especially with regard to \u0026amp;#39;t Hooft\u0026amp;#39;s criterion of naturalness. It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. There are two solutions to this problem: (i) a global supersymmetry, which ensures the absence of all","publication_date":{"day":null,"month":null,"year":1983,"errors":{}},"publication_name":"Reviews of Modern Physics"},"translated_abstract":"The need for reexamination of the standard model of strong, weak, and electromagnetic interactions is discussed, especially with regard to \u0026amp;#39;t Hooft\u0026amp;#39;s criterion of naturalness. It has been argued that theories with fundamental scalar fields tend to be unnatural at relatively low energies. 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