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<span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjqt/s40507-022-00147-w">10.1140/epjqt/s40507-022-00147-w <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Alonso%2C+I">Ivan Alonso</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alpigiani%2C+C">Cristiano Alpigiani</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Altschul%2C+B">Brett Altschul</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Araujo%2C+H">Henrique Araujo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arduini%2C+G">Gianluigi Arduini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arlt%2C+J">Jan Arlt</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Badurina%2C+L">Leonardo Badurina</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Balaz%2C+A">Antun Balaz</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bandarupally%2C+S">Satvika Bandarupally</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barone%2C+B+C+B+M">Barry C Barish Michele Barone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barsanti%2C+M">Michele Barsanti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bass%2C+S">Steven Bass</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bassi%2C+A">Angelo Bassi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Battelier%2C+B">Baptiste Battelier</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baynham%2C+C+F+A">Charles F. A. Baynham</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Beaufils%2C+Q">Quentin Beaufils</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Belic%2C+A">Aleksandar Belic</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Berge%2C+J">Joel Berge</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bernabeu%2C+J">Jose Bernabeu</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bertoldi%2C+A">Andrea Bertoldi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bingham%2C+R">Robert Bingham</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bize%2C+S">Sebastien Bize</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Blas%2C+D">Diego Blas</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bongs%2C+K">Kai Bongs</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bouyer%2C+P">Philippe Bouyer</a> , et al. (224 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2201.07789v1-abstract-short" style="display: inline;"> We summarize the discussions at a virtual Community Workshop on Cold Atoms in Space concerning the status of cold atom technologies, the prospective scientific and societal opportunities offered by their deployment in space, and the developments needed before cold atoms could be operated in space. The cold atom technologies discussed include atomic clocks, quantum gravimeters and accelerometers, a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2201.07789v1-abstract-full').style.display = 'inline'; document.getElementById('2201.07789v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2201.07789v1-abstract-full" style="display: none;"> We summarize the discussions at a virtual Community Workshop on Cold Atoms in Space concerning the status of cold atom technologies, the prospective scientific and societal opportunities offered by their deployment in space, and the developments needed before cold atoms could be operated in space. The cold atom technologies discussed include atomic clocks, quantum gravimeters and accelerometers, and atom interferometers. Prospective applications include metrology, geodesy and measurement of terrestrial mass change due to, e.g., climate change, and fundamental science experiments such as tests of the equivalence principle, searches for dark matter, measurements of gravitational waves and tests of quantum mechanics. We review the current status of cold atom technologies and outline the requirements for their space qualification, including the development paths and the corresponding technical milestones, and identifying possible pathfinder missions to pave the way for missions to exploit the full potential of cold atoms in space. Finally, we present a first draft of a possible road-map for achieving these goals, that we propose for discussion by the interested cold atom, Earth Observation, fundamental physics and other prospective scientific user communities, together with ESA and national space and research funding agencies. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2201.07789v1-abstract-full').style.display = 'none'; document.getElementById('2201.07789v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 January, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Summary of the Community Workshop on Cold Atoms in Space and corresponding Road-map: https://indico.cern.ch/event/1064855/</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> EPJ Quantum Technol. 9, 30 (2022) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1701.06902">arXiv:1701.06902</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1701.06902">pdf</a>, <a href="https://arxiv.org/ps/1701.06902">ps</a>, <a href="https://arxiv.org/format/1701.06902">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Improved Tests of Lorentz Invariance in the Matter Sector using Atomic Clocks </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Bars%2C+H+P">H. Pihan-Le Bars</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guerlin%2C+C">C. Guerlin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bailey%2C+Q+G">Q. G. Bailey</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bize%2C+S">S. Bize</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Wolf%2C+P">P. Wolf</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1701.06902v1-abstract-short" style="display: inline;"> For the purpose of searching for Lorentz-invariance violation in the minimal Standard-Model Extension, we perfom a reanalysis of data obtained from the $^{133}\text{Cs}$ fountain clock operating at SYRTE. The previous study led to new limits on eight components of the $\tilde{c}_{渭谓}$ tensor, which quantifies the anisotropy of the proton kinetic energy. We recently derived an advanced model for th&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1701.06902v1-abstract-full').style.display = 'inline'; document.getElementById('1701.06902v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1701.06902v1-abstract-full" style="display: none;"> For the purpose of searching for Lorentz-invariance violation in the minimal Standard-Model Extension, we perfom a reanalysis of data obtained from the $^{133}\text{Cs}$ fountain clock operating at SYRTE. The previous study led to new limits on eight components of the $\tilde{c}_{渭谓}$ tensor, which quantifies the anisotropy of the proton kinetic energy. We recently derived an advanced model for the frequency shift of hyperfine Zeeman transition due to Lorentz violation and became able to constrain the ninth component, the isotropic coefficient $\tilde{c}_{TT}$, which is the least well-constrained coefficient of $\tilde{c}_{渭谓}$. This model is based on a second-order boost Lorentz transformation from the laboratory frame to the Sun-centered frame, and it gives rise to an improvement of five orders of magnitude on $\tilde{c}_{TT}$ compared to the state of the art. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1701.06902v1-abstract-full').style.display = 'none'; document.getElementById('1701.06902v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 January, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2017. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1612.07390">arXiv:1612.07390</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1612.07390">pdf</a>, <a href="https://arxiv.org/format/1612.07390">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.95.075026">10.1103/PhysRevD.95.075026 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Lorentz-symmetry test at Planck-scale suppression with nucleons in a spin-polarized $^{133}$Cs cold atom clock </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Bars%2C+H+P">H. Pihan-Le Bars</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guerlin%2C+C">C. Guerlin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Lasseri%2C+R+-">R. -D. Lasseri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ebran%2C+J+-">J. -P. Ebran</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bailey%2C+Q+G">Q. G. Bailey</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bize%2C+S">S. Bize</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Khan%2C+E">E. Khan</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Wolf%2C+P">P. Wolf</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1612.07390v2-abstract-short" style="display: inline;"> We introduce an improved model that links the frequency shift of the $^{133}\text{Cs}$ hyperfine Zeeman transitions $\vert F = 3, m_F&gt; \longleftrightarrow \vert F = 4, m_F &gt;$ to the Lorentz-violating Standard-Model Extension (SME) coefficients of the proton and neutron. The new model uses Lorentz transformations developed to second order in boost and additionally takes the nuclear structure into a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.07390v2-abstract-full').style.display = 'inline'; document.getElementById('1612.07390v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1612.07390v2-abstract-full" style="display: none;"> We introduce an improved model that links the frequency shift of the $^{133}\text{Cs}$ hyperfine Zeeman transitions $\vert F = 3, m_F&gt; \longleftrightarrow \vert F = 4, m_F &gt;$ to the Lorentz-violating Standard-Model Extension (SME) coefficients of the proton and neutron. The new model uses Lorentz transformations developed to second order in boost and additionally takes the nuclear structure into account, beyond the simple Schmidt model used previously in SME analyses, thereby providing access to both proton and neutron SME coefficients including the isotropic coefficient $\tilde{c}_{TT}$. Using this new model in a second analysis of the data delivered by the FO2 dual Cs/Rb fountain at Paris Observatory and previously analysed in arXiv:hep-ph/0601024v1, we improve by up to 12 orders of magnitude the present maximum sensitivities (see arXiv:0801.0287v9) on the $\tilde{c}_{Q}$, $\tilde{c}_{TJ}$ and $\tilde{c}_{TT}$ coefficients for the neutron and on the $\tilde{c}_{TT}$ coefficient for the proton, reaching respectively $10^{-20}$, $10^{-17}$, $10^{-13}$ and $10^{-15}$ GeV. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.07390v2-abstract-full').style.display = 'none'; document.getElementById('1612.07390v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 May, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 December, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 95, 075026 (2017) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0212112">arXiv:physics/0212112</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0212112">pdf</a>, <a href="https://arxiv.org/ps/physics/0212112">ps</a>, <a href="https://arxiv.org/format/physics/0212112">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.90.150801">10.1103/PhysRevLett.90.150801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Search for Variations of Fundamental Constants using Atomic Fountain Clocks </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Marion%2C+H">H. Marion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Santos%2C+F+P+D">F. Pereira Dos Santos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Abgrall%2C+M">M. Abgrall</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Zhang%2C+S">S. Zhang</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Sortais%2C+Y">Y. Sortais</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bize%2C+S">S. Bize</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Maksimovic%2C+I">I. Maksimovic</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calonico%2C+D">D. Calonico</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gruenert%2C+J">J. Gruenert</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Mandache%2C+C">C. Mandache</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Lemonde%2C+P">P. Lemonde</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Santarelli%2C+G">G. Santarelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Laurent%2C+P">Ph. Laurent</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Clairon%2C+A">A. Clairon</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Salomon%2C+C">C. Salomon</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="physics/0212112v1-abstract-short" style="display: inline;"> Over five years we have compared the hyperfine frequencies of 133Cs and 87Rb atoms in their electronic ground state using several laser cooled 133Cs and 87Rb atomic fountains with an accuracy of ~10^{-15}. These measurements set a stringent upper bound to a possible fractional time variation of the ratio between the two frequencies : (d/dt)ln(nu_Rb/nu_Cs)=(0.2 +/- 7.0)*10^{-16} yr^{-1} (1 sigma&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0212112v1-abstract-full').style.display = 'inline'; document.getElementById('physics/0212112v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0212112v1-abstract-full" style="display: none;"> Over five years we have compared the hyperfine frequencies of 133Cs and 87Rb atoms in their electronic ground state using several laser cooled 133Cs and 87Rb atomic fountains with an accuracy of ~10^{-15}. These measurements set a stringent upper bound to a possible fractional time variation of the ratio between the two frequencies : (d/dt)ln(nu_Rb/nu_Cs)=(0.2 +/- 7.0)*10^{-16} yr^{-1} (1 sigma uncertainty). The same limit applies to a possible variation of the quantity (mu_Rb/mu_Cs)*alpha^{-0.44}, which involves the ratio of nuclear magnetic moments and the fine structure constant. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0212112v1-abstract-full').style.display = 'none'; document.getElementById('physics/0212112v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 December, 2002; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2002. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">4 pages, 3 figures, 1 table submitted to Phys. Rev. Lett</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett. 90 (2003) 150801 </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 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