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is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/epjc/s10052-023-12137-y">10.1140/epjc/s10052-023-12137-y <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Production of antihydrogen atoms by 6 keV antiprotons through a positronium cloud </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/physics?searchtype=author&amp;query=Blumer%2C+P">P. Blumer</a>, <a href="/search/physics?searchtype=author&amp;query=Caratsch%2C+G">G. Caratsch</a>, <a href="/search/physics?searchtype=author&amp;query=Chung%2C+M">M. Chung</a>, <a href="/search/physics?searchtype=author&amp;query=Clad%C3%A9%2C+P">P. Clad茅</a>, <a href="/search/physics?searchtype=author&amp;query=Comini%2C+P">P. Comini</a>, <a href="/search/physics?searchtype=author&amp;query=Crivelli%2C+P">P. Crivelli</a>, <a href="/search/physics?searchtype=author&amp;query=Dalkarov%2C+O">O. Dalkarov</a>, <a href="/search/physics?searchtype=author&amp;query=Debu%2C+P">P. Debu</a>, <a href="/search/physics?searchtype=author&amp;query=Douillet%2C+A">A. Douillet</a>, <a href="/search/physics?searchtype=author&amp;query=Drapier%2C+D">D. Drapier</a>, <a href="/search/physics?searchtype=author&amp;query=Froelich%2C+P">P. Froelich</a>, <a href="/search/physics?searchtype=author&amp;query=Garroum%2C+N">N. Garroum</a>, <a href="/search/physics?searchtype=author&amp;query=Guellati-Khelifa%2C+S">S. Guellati-Khelifa</a>, <a href="/search/physics?searchtype=author&amp;query=Guyomard%2C+J">J. Guyomard</a>, <a href="/search/physics?searchtype=author&amp;query=Hervieux%2C+P">P-A. Hervieux</a>, <a href="/search/physics?searchtype=author&amp;query=Hilico%2C+L">L. Hilico</a>, <a href="/search/physics?searchtype=author&amp;query=Indelicato%2C+P">P. Indelicato</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Karr%2C+J">J-P. Karr</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+B">B. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+S">S. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+E">E-S. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Ko%2C+Y+J">Y. J. Ko</a>, <a href="/search/physics?searchtype=author&amp;query=Kosinski%2C+T">T. Kosinski</a> , et al. (39 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="2306.15801v2-abstract-short" style="display: inline;"> We report on the first production of an antihydrogen beam by charge exchange of 6.1 keV antiprotons with a cloud of positronium in the GBAR experiment at CERN. The antiproton beam was delivered by the AD/ELENA facility. The positronium target was produced from a positron beam itself obtained from an electron linear accelerator. We observe an excess over background indicating antihydrogen productio&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2306.15801v2-abstract-full').style.display = 'inline'; document.getElementById('2306.15801v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2306.15801v2-abstract-full" style="display: none;"> We report on the first production of an antihydrogen beam by charge exchange of 6.1 keV antiprotons with a cloud of positronium in the GBAR experiment at CERN. The antiproton beam was delivered by the AD/ELENA facility. The positronium target was produced from a positron beam itself obtained from an electron linear accelerator. We observe an excess over background indicating antihydrogen production with a significance of 3-4 standard deviations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2306.15801v2-abstract-full').style.display = 'none'; document.getElementById('2306.15801v2-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> 3 July, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 June, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> European Physical Journal C 83, 1004 (2023) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2304.00878">arXiv:2304.00878</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2304.00878">pdf</a>, <a href="https://arxiv.org/format/2304.00878">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> </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/PhysRevA.107.053319">10.1103/PhysRevA.107.053319 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A multichannel hyperspherical model for Efimov physics with van der Waals interactions controlled by a Feshbach resonance </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Tempest%2C+K">Kajsa-My Tempest</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</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="2304.00878v1-abstract-short" style="display: inline;"> Here we present a four-channel model that incorporates a magnetically tunable Feshbach resonance in a system of three atoms that interact via pairwise van der Waals interactions. Our method is designed to model recent experiments where the tunability of the scattering length has been used to study three-body Efimov states, which appear in the limit of a diverging two-body scattering length. Using&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.00878v1-abstract-full').style.display = 'inline'; document.getElementById('2304.00878v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2304.00878v1-abstract-full" style="display: none;"> Here we present a four-channel model that incorporates a magnetically tunable Feshbach resonance in a system of three atoms that interact via pairwise van der Waals interactions. Our method is designed to model recent experiments where the tunability of the scattering length has been used to study three-body Efimov states, which appear in the limit of a diverging two-body scattering length. Using this model, we calculate three-body adiabatic and effective potential curves and study how the strength (or width) of the Feshbach resonance affects the three-body potential that is connected to the Efimov effect. We find that the position of the repulsive barrier, which has been used to explain the so-called van der Waals universality in broad resonances, is slightly shifted as the narrow resonance limit is approached and that this shift is correlated to the appearance of two avoided crossings in the adiabatic energy landscape. More importantly, the attractive well is markedly shifted upward in energy and is extremely shallow for the narrowest resonance. We argue that this behavior is connected to the breakdown of van der Waals universality for weak (narrow) resonances. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.00878v1-abstract-full').style.display = 'none'; document.getElementById('2304.00878v1-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> 3 April, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2023. </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">23 pages, 12 figures, submitted to Physical Review A</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2205.04530">arXiv:2205.04530</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2205.04530">pdf</a>, <a href="https://arxiv.org/format/2205.04530">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-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/10.1016/j.nima.2022.167263">10.1016/j.nima.2022.167263 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Positron accumulation in the GBAR experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Blumer%2C+P">P. Blumer</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Chung%2C+M">M. Chung</a>, <a href="/search/physics?searchtype=author&amp;query=Clade%2C+P">P. Clade</a>, <a href="/search/physics?searchtype=author&amp;query=Comini%2C+P">P. Comini</a>, <a href="/search/physics?searchtype=author&amp;query=Crivelli%2C+P">P. Crivelli</a>, <a href="/search/physics?searchtype=author&amp;query=Dalkarov%2C+O">O. Dalkarov</a>, <a href="/search/physics?searchtype=author&amp;query=Debu%2C+P">P. Debu</a>, <a href="/search/physics?searchtype=author&amp;query=Dodd%2C+L">L. Dodd</a>, <a href="/search/physics?searchtype=author&amp;query=Douillet%2C+A">A. Douillet</a>, <a href="/search/physics?searchtype=author&amp;query=Guellati%2C+S">S. Guellati</a>, <a href="/search/physics?searchtype=author&amp;query=Hervieux%2C+P+-">P. -A Hervieux</a>, <a href="/search/physics?searchtype=author&amp;query=Hilico%2C+L">L. Hilico</a>, <a href="/search/physics?searchtype=author&amp;query=Indelicato%2C+P">P. Indelicato</a>, <a href="/search/physics?searchtype=author&amp;query=Janka%2C+G">G. Janka</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Karr%2C+J+-">J. -P. Karr</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+B+H">B. H. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+E+S">E. S. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+S+K">S. K. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Ko%2C+Y">Y. Ko</a>, <a href="/search/physics?searchtype=author&amp;query=Kosinski%2C+T">T. Kosinski</a>, <a href="/search/physics?searchtype=author&amp;query=Kuroda%2C+N">N. Kuroda</a>, <a href="/search/physics?searchtype=author&amp;query=Latacz%2C+B+M">B. M. Latacz</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+B">B. Lee</a> , et al. (45 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="2205.04530v1-abstract-short" style="display: inline;"> We present a description of the GBAR positron (e+) trapping apparatus, which consists of a three stage Buffer Gas Trap (BGT) followed by a High Field Penning Trap (HFT), and discuss its performance. The overall goal of the GBAR experiment is to measure the acceleration of the neutral antihydrogen (H) atom in the terrestrial gravitational field by neutralising a positive antihydrogen ion (H+), whic&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.04530v1-abstract-full').style.display = 'inline'; document.getElementById('2205.04530v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2205.04530v1-abstract-full" style="display: none;"> We present a description of the GBAR positron (e+) trapping apparatus, which consists of a three stage Buffer Gas Trap (BGT) followed by a High Field Penning Trap (HFT), and discuss its performance. The overall goal of the GBAR experiment is to measure the acceleration of the neutral antihydrogen (H) atom in the terrestrial gravitational field by neutralising a positive antihydrogen ion (H+), which has been cooled to a low temperature, and observing the subsequent H annihilation following free fall. To produce one H+ ion, about 10^10 positrons, efficiently converted into positronium (Ps), together with about 10^7 antiprotons (p), are required. The positrons, produced from an electron linac-based system, are accumulated first in the BGT whereafter they are stacked in the ultra-high vacuum HFT, where we have been able to trap 1.4(2) x 10^9 positrons in 1100 seconds. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.04530v1-abstract-full').style.display = 'none'; document.getElementById('2205.04530v1-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> 9 May, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Instruments and Methods in Physics Research Section A, Volume 1040, 2022, 167263 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2107.08152">arXiv:2107.08152</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2107.08152">pdf</a>, <a href="https://arxiv.org/format/2107.08152">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> </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/10.1007/s10751-016-1382-6">10.1007/s10751-016-1382-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Limit on the Electric Charge of Antihydrogen </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Capra%2C+A">A. Capra</a>, <a href="/search/physics?searchtype=author&amp;query=Amole%2C+C">C. Amole</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Eriksson%2C+S">S. Eriksson</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Gutierrez%2C+A">A. Gutierrez</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Isaac%2C+C+A">C. A. Isaac</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L+.">L . Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Little%2C+A">A. Little</a>, <a href="/search/physics?searchtype=author&amp;query=McKenna%2C+J+T+K">J. T. K. McKenna</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">S. Menary</a>, <a href="/search/physics?searchtype=author&amp;query=Napoli%2C+S+C">S. C. Napoli</a>, <a href="/search/physics?searchtype=author&amp;query=Nolan%2C+P">P. Nolan</a> , et al. (15 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="2107.08152v1-abstract-short" style="display: inline;"> The ALPHA collaboration has successfully demonstrated the production and the confinement of cold antihydrogen, $\overline{\mathrm{H}}$. An analysis of trapping data allowed a stringent limit to be placed on the electric charge of the simplest antiatom. Charge neutrality of matter is known to a very high precision, hence a neutrality limit of $\overline{\mathrm{H}}$ provides a test of CPT invarianc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.08152v1-abstract-full').style.display = 'inline'; document.getElementById('2107.08152v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2107.08152v1-abstract-full" style="display: none;"> The ALPHA collaboration has successfully demonstrated the production and the confinement of cold antihydrogen, $\overline{\mathrm{H}}$. An analysis of trapping data allowed a stringent limit to be placed on the electric charge of the simplest antiatom. Charge neutrality of matter is known to a very high precision, hence a neutrality limit of $\overline{\mathrm{H}}$ provides a test of CPT invariance. The experimental technique is based on the measurement of the deflection of putatively charged $\overline{\mathrm{H}}$ in an electric field. The tendency for trapped $\overline{\mathrm{H}}$ atoms to be displaced by electrostatic fields is measured and compared to the results of a detailed simulation of $\overline{\mathrm{H}}$ dynamics in the trap. An extensive survey of the systematic errors is performed, with particular attention to those due to the silicon vertex detector, which is the device used to determine the $\overline{\mathrm{H}}$ annihilation position. The limit obtained on the charge of the $\overline{\mathrm{H}}$ atom is \mbox{$ Q = (-1.3\pm1.8\pm0.4)\times10^{-8}$}, representing the first precision measurement with $\overline{\mathrm{H}}$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.08152v1-abstract-full').style.display = 'none'; document.getElementById('2107.08152v1-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> 16 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2021. </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">5 pages, 3 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Hyperfine Interact 238, 9 (2017) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2006.05966">arXiv:2006.05966</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2006.05966">pdf</a>, <a href="https://arxiv.org/format/2006.05966">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.1016/j.nima.2020.164657">10.1016/j.nima.2020.164657 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Positron production using a 9 MeV electron linac for the GBAR experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Choi%2C+J+J">J. J. Choi</a>, <a href="/search/physics?searchtype=author&amp;query=Chung%2C+M">M. Chung</a>, <a href="/search/physics?searchtype=author&amp;query=Clade%2C+P">P. Clade</a>, <a href="/search/physics?searchtype=author&amp;query=Comini%2C+P">P. Comini</a>, <a href="/search/physics?searchtype=author&amp;query=Crepin%2C+P">P-P. Crepin</a>, <a href="/search/physics?searchtype=author&amp;query=Crivelli%2C+P">P. Crivelli</a>, <a href="/search/physics?searchtype=author&amp;query=Dalkarov%2C+O">O. Dalkarov</a>, <a href="/search/physics?searchtype=author&amp;query=Debu%2C+P">P. Debu</a>, <a href="/search/physics?searchtype=author&amp;query=Dodd%2C+L">L. Dodd</a>, <a href="/search/physics?searchtype=author&amp;query=Douillet%2C+A">A. Douillet</a>, <a href="/search/physics?searchtype=author&amp;query=Guellati-Khelifa%2C+S">S. Guellati-Khelifa</a>, <a href="/search/physics?searchtype=author&amp;query=Hervieux%2C+P">P-A. Hervieux</a>, <a href="/search/physics?searchtype=author&amp;query=Hilico%2C+L">L. Hilico</a>, <a href="/search/physics?searchtype=author&amp;query=Husson%2C+A">A. Husson</a>, <a href="/search/physics?searchtype=author&amp;query=Indelicato%2C+P">P. Indelicato</a>, <a href="/search/physics?searchtype=author&amp;query=Janka%2C+G">G. Janka</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Karr%2C+J">J-P. Karr</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+B+H">B. H. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+E">E-S. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Kim%2C+S+K">S. K. Kim</a>, <a href="/search/physics?searchtype=author&amp;query=Ko%2C+Y">Y. Ko</a>, <a href="/search/physics?searchtype=author&amp;query=Kosinski%2C+T">T. Kosinski</a>, <a href="/search/physics?searchtype=author&amp;query=Kuroda%2C+N">N. Kuroda</a> , et al. (45 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="2006.05966v3-abstract-short" style="display: inline;"> For the GBAR (Gravitational Behaviour of Antihydrogen at Rest) experiment at CERN&#39;s Antiproton Decelerator (AD) facility we have constructed a source of slow positrons, which uses a low-energy electron linear accelerator (linac). The driver linac produces electrons of 9 MeV kinetic energy that create positrons from bremsstrahlung-induced pair production. Staying below 10 MeV ensures no persistent&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.05966v3-abstract-full').style.display = 'inline'; document.getElementById('2006.05966v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2006.05966v3-abstract-full" style="display: none;"> For the GBAR (Gravitational Behaviour of Antihydrogen at Rest) experiment at CERN&#39;s Antiproton Decelerator (AD) facility we have constructed a source of slow positrons, which uses a low-energy electron linear accelerator (linac). The driver linac produces electrons of 9 MeV kinetic energy that create positrons from bremsstrahlung-induced pair production. Staying below 10 MeV ensures no persistent radioactive activation in the target zone and that the radiation level outside the biological shield is safe for public access. An annealed tungsten-mesh assembly placed directly behind the target acts as a positron moderator. The system produces $5\times10^7$ slow positrons per second, a performance demonstrating that a low-energy electron linac is a superior choice over positron-emitting radioactive sources for high positron flux. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.05966v3-abstract-full').style.display = 'none'; document.getElementById('2006.05966v3-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> 6 October, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 10 June, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2020. </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">published in NIM A. 33 pages 9 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl. Instrum. Methods Phys. Res. A 985, 164657 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1808.10230">arXiv:1808.10230</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1808.10230">pdf</a>, <a href="https://arxiv.org/format/1808.10230">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> </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/10.1098/rsta.2017.0271">10.1098/rsta.2017.0271 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Collisions involving antiprotons and antihydrogen: an overview </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</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="1808.10230v1-abstract-short" style="display: inline;"> I give an overview of experimental and theoretical results for antiproton and antihydrogen scattering with atoms and molecules (in particular H, He). At low energies ($\lesssim1$~keV) there are practically no experimental data available. Instead I compare the results from different theoretical calculations, of various degrees of sophistication. At energies up to a few 10:s of eV, I focus on simple&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10230v1-abstract-full').style.display = 'inline'; document.getElementById('1808.10230v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1808.10230v1-abstract-full" style="display: none;"> I give an overview of experimental and theoretical results for antiproton and antihydrogen scattering with atoms and molecules (in particular H, He). At low energies ($\lesssim1$~keV) there are practically no experimental data available. Instead I compare the results from different theoretical calculations, of various degrees of sophistication. At energies up to a few 10:s of eV, I focus on simple approximations that give reasonably accurate results, as these allow quick estimates of collision rates without embarking on a research project. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10230v1-abstract-full').style.display = 'none'; document.getElementById('1808.10230v1-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> 30 August, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2018. </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">13 pages, 9 figures. This article is part of the Theo Murphy meeting issue &#34;Antiproton physics in the ELENA era&#34;</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phil. Trans. R. Soc. A 376: 2017027 2018 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1604.03374">arXiv:1604.03374</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1604.03374">pdf</a>, <a href="https://arxiv.org/format/1604.03374">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> </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/PhysRevA.93.053416">10.1103/PhysRevA.93.053416 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Bimodal momentum distribution of laser-cooled atoms in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">Claude M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">Anders Kastberg</a>, <a href="/search/physics?searchtype=author&amp;query=Sj%C3%B6lund%2C+P">Peder Sj枚lund</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="1604.03374v2-abstract-short" style="display: inline;"> We study, numerically and experimentally, the momentum distribution of atoms cooled in optical lattices. Using semi-classical simulations, we show that this distribution is bimodal, made up of a central feature corresponding to &#34;cold&#34;, trapped atoms, with tails of &#34;hot&#34;, untrapped atoms, and that this holds true also for very shallow potentials. Careful analysis of the distribution of high-momentu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.03374v2-abstract-full').style.display = 'inline'; document.getElementById('1604.03374v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1604.03374v2-abstract-full" style="display: none;"> We study, numerically and experimentally, the momentum distribution of atoms cooled in optical lattices. Using semi-classical simulations, we show that this distribution is bimodal, made up of a central feature corresponding to &#34;cold&#34;, trapped atoms, with tails of &#34;hot&#34;, untrapped atoms, and that this holds true also for very shallow potentials. Careful analysis of the distribution of high-momentum untrapped atoms, both from simulations and experiments, shows that the tails of the distribution does not follow a normal law, hinting at a power-law distribution and non-ergodic behavior. We also revisit the phenomenon of d茅crochage, the potential depth below which the temperature of the atoms starts increasing. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1604.03374v2-abstract-full').style.display = 'none'; document.getElementById('1604.03374v2-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> 15 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. A 93, 053416 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1405.0692">arXiv:1405.0692</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1405.0692">pdf</a>, <a href="https://arxiv.org/ps/1405.0692">ps</a>, <a href="https://arxiv.org/format/1405.0692">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</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/10.1088/1367-2630/16/1/013037">10.1088/1367-2630/16/1/013037 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> In situ electromagnetic field diagnostics with an electron plasma in a Penning-Malmberg trap </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Amole%2C+C">C. Amole</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Capra%2C+A">A. Capra</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Deller%2C+A">A. Deller</a>, <a href="/search/physics?searchtype=author&amp;query=Evetts%2C+N">N. Evetts</a>, <a href="/search/physics?searchtype=author&amp;query=Eriksson%2C+S">S. Eriksson</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Gutierrez%2C+A">A. Gutierrez</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Isaac%2C+C+A">C. A. Isaac</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">L. Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Little%2C+A">A. Little</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=McKenna%2C+J+T+K">J. T. K. McKenna</a> , et al. (15 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="1405.0692v1-abstract-short" style="display: inline;"> We demonstrate a novel detection method for the cyclotron resonance frequency of an electron plasma in a Penning-Malmberg trap. With this technique, the electron plasma is used as an in situ diagnostic tool for measurement of the static magnetic field and the microwave electric field in the trap. The cyclotron motion of the electron plasma is excited by microwave radiation and the temperature chan&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1405.0692v1-abstract-full').style.display = 'inline'; document.getElementById('1405.0692v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1405.0692v1-abstract-full" style="display: none;"> We demonstrate a novel detection method for the cyclotron resonance frequency of an electron plasma in a Penning-Malmberg trap. With this technique, the electron plasma is used as an in situ diagnostic tool for measurement of the static magnetic field and the microwave electric field in the trap. The cyclotron motion of the electron plasma is excited by microwave radiation and the temperature change of the plasma is measured non-destructively by monitoring the plasma&#39;s quadrupole mode frequency. The spatially-resolved microwave electric field strength can be inferred from the plasma temperature change and the magnetic field is found through the cyclotron resonance frequency. These measurements were used extensively in the recently reported demonstration of resonant quantum interactions with antihydrogen. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1405.0692v1-abstract-full').style.display = 'none'; document.getElementById('1405.0692v1-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> 4 May, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2014. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> New J. Phys. 16 013037 (2014) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1201.3944">arXiv:1201.3944</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1201.3944">pdf</a>, <a href="https://arxiv.org/format/1201.3944">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="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-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/10.1088/1367-2630/14/1/015010.">10.1088/1367-2630/14/1/015010. <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Antihydrogen and mirror-trapped antiproton discrimination: Discriminating between antihydrogen and mirror-trapped antiprotons in a minimum-B trap </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Amole%2C+C">C. Amole</a>, <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">G. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">S. Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Deller%2C+A">A. Deller</a>, <a href="/search/physics?searchtype=author&amp;query=Eriksson%2C+S">S. Eriksson</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Gutierrez%2C+A">A. Gutierrez</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">A. J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">R. Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">L. Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">S. Menary</a> , et al. (13 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="1201.3944v1-abstract-short" style="display: inline;"> Recently, antihydrogen atoms were trapped at CERN in a magnetic minimum (minimum-B) trap formed by superconducting octupole and mirror magnet coils. The trapped antiatoms were detected by rapidly turning off these magnets, thereby eliminating the magnetic minimum and releasing any antiatoms contained in the trap. Once released, these antiatoms quickly hit the trap wall, whereupon the positrons and&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1201.3944v1-abstract-full').style.display = 'inline'; document.getElementById('1201.3944v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1201.3944v1-abstract-full" style="display: none;"> Recently, antihydrogen atoms were trapped at CERN in a magnetic minimum (minimum-B) trap formed by superconducting octupole and mirror magnet coils. The trapped antiatoms were detected by rapidly turning off these magnets, thereby eliminating the magnetic minimum and releasing any antiatoms contained in the trap. Once released, these antiatoms quickly hit the trap wall, whereupon the positrons and antiprotons in the antiatoms annihilated. The antiproton annihilations produce easily detected signals; we used these signals to prove that we trapped antihydrogen. However, our technique could be confounded by mirror-trapped antiprotons, which would produce seemingly-identical annihilation signals upon hitting the trap wall. In this paper, we discuss possible sources of mirror-trapped antiprotons and show that antihydrogen and antiprotons can be readily distinguished, often with the aid of applied electric fields, by analyzing the annihilation locations and times. We further discuss the general properties of antiproton and antihydrogen trajectories in this magnetic geometry, and reconstruct the antihydrogen energy distribution from the measured annihilation time history. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1201.3944v1-abstract-full').style.display = 'none'; document.getElementById('1201.3944v1-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> 18 January, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2012. </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">17 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> New J. Phys., 14 015010, 2012 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1105.0037">arXiv:1105.0037</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1105.0037">pdf</a>, <a href="https://arxiv.org/ps/1105.0037">ps</a>, <a href="https://arxiv.org/format/1105.0037">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="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-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/10.1007/s10751-011-0299-3">10.1007/s10751-011-0299-3 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Towards Antihydrogen Trapping and Spectroscopy at ALPHA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">Eoin Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">Gorm. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">Mohammad. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">Marcelo Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">William Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Bowe%2C+P+D">Paul D. Bowe</a>, <a href="/search/physics?searchtype=author&amp;query=Bray%2C+C+C">Crystal C. Bray</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">Claudio L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">Steven Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">Michael Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">Joel Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">Tim Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">Makoto C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">David R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">Jeffrey S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">Walter N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">Ruyugo S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">Michael E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">Andrew J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">Richard Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">Leonid Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Lambo%2C+R">Ricardo Lambo</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">Niels Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">Scott Menary</a> , et al. (15 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="1105.0037v1-abstract-short" style="display: inline;"> Spectroscopy of antihydrogen has the potential to yield high-precision tests of the CPT theorem and shed light on the matter-antimatter imbalance in the Universe. The ALPHA antihydrogen trap at CERN&#39;s Antiproton Decelerator aims to prepare a sample of antihydrogen atoms confined in an octupole-based Ioffe trap and to measure the frequency of several atomic transitions. We describe our techniques t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.0037v1-abstract-full').style.display = 'inline'; document.getElementById('1105.0037v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1105.0037v1-abstract-full" style="display: none;"> Spectroscopy of antihydrogen has the potential to yield high-precision tests of the CPT theorem and shed light on the matter-antimatter imbalance in the Universe. The ALPHA antihydrogen trap at CERN&#39;s Antiproton Decelerator aims to prepare a sample of antihydrogen atoms confined in an octupole-based Ioffe trap and to measure the frequency of several atomic transitions. We describe our techniques to directly measure the antiproton temperature and a new technique to cool them to below 10 K. We also show how our unique position-sensitive annihilation detector provides us with a highly sensitive method of identifying antiproton annihilations and effectively rejecting the cosmic-ray background. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.0037v1-abstract-full').style.display = 'none'; document.getElementById('1105.0037v1-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> 29 April, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2011. </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">10 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1104.4982">arXiv:1104.4982</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1104.4982">pdf</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="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="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-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/10.1038/nphys2025">10.1038/nphys2025 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Confinement of antihydrogen for 1000 seconds </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=ALPHA+Collaboration"> ALPHA Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">G. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Deller%2C+A">A. Deller</a>, <a href="/search/physics?searchtype=author&amp;query=Eriksson%2C+S">S. Eriksson</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Gutierrez%2C+A">A. Gutierrez</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">R. S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">A. J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">R. Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kemp%2C+S">S. Kemp</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">L. Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">S. Menary</a> , et al. (14 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="1104.4982v1-abstract-short" style="display: inline;"> Atoms made of a particle and an antiparticle are unstable, usually surviving less than a microsecond. Antihydrogen, made entirely of antiparticles, is believed to be stable, and it is this longevity that holds the promise of precision studies of matter-antimatter symmetry. We have recently demonstrated trapping of antihydrogen atoms by releasing them after a confinement time of 172 ms. A critical&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1104.4982v1-abstract-full').style.display = 'inline'; document.getElementById('1104.4982v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1104.4982v1-abstract-full" style="display: none;"> Atoms made of a particle and an antiparticle are unstable, usually surviving less than a microsecond. Antihydrogen, made entirely of antiparticles, is believed to be stable, and it is this longevity that holds the promise of precision studies of matter-antimatter symmetry. We have recently demonstrated trapping of antihydrogen atoms by releasing them after a confinement time of 172 ms. A critical question for future studies is: how long can anti-atoms be trapped? Here we report the observation of anti-atom confinement for 1000 s, extending our earlier results by nearly four orders of magnitude. Our calculations indicate that most of the trapped anti-atoms reach the ground state. Further, we report the first measurement of the energy distribution of trapped antihydrogen which, coupled with detailed comparisons with simulations, provides a key tool for the systematic investigation of trapping dynamics. These advances open up a range of experimental possibilities, including precision studies of CPT symmetry and cooling to temperatures where gravitational effects could become apparent. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1104.4982v1-abstract-full').style.display = 'none'; document.getElementById('1104.4982v1-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> 26 April, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2011. </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">30 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> TRI-PP-11-02 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nature Phys.7:558-564,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1104.4841">arXiv:1104.4841</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1104.4841">pdf</a>, <a href="https://arxiv.org/format/1104.4841">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-ph</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="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/10.1103/PhysRevLett.106.145001">10.1103/PhysRevLett.106.145001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Centrifugal separation and equilibration dynamics in an electron-antiproton plasma </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">G. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Bowe%2C+P+D">P. D. Bowe</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">S. Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Deller%2C+A">A. Deller</a>, <a href="/search/physics?searchtype=author&amp;query=Eriksson%2C+S">S. Eriksson</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Gutierrez%2C+A">A. Gutierrez</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">A. J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">R. Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">S. Menary</a>, <a href="/search/physics?searchtype=author&amp;query=Nolan%2C+P">P. Nolan</a> , et al. (12 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="1104.4841v1-abstract-short" style="display: inline;"> Charges in cold, multiple-species, non-neutral plasmas separate radially by mass, forming centrifugally-separated states. Here, we report the first detailed measurements of such states in an electron-antiproton plasma, and the first observations of the separation dynamics in any centrifugally-separated system. While the observed equilibrium states are expected and in agreement with theory, the equ&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1104.4841v1-abstract-full').style.display = 'inline'; document.getElementById('1104.4841v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1104.4841v1-abstract-full" style="display: none;"> Charges in cold, multiple-species, non-neutral plasmas separate radially by mass, forming centrifugally-separated states. Here, we report the first detailed measurements of such states in an electron-antiproton plasma, and the first observations of the separation dynamics in any centrifugally-separated system. While the observed equilibrium states are expected and in agreement with theory, the equilibration time is approximately constant over a wide range of parameters, a surprising and as yet unexplained result. Electron-antiproton plasmas play a crucial role in antihydrogen trapping experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1104.4841v1-abstract-full').style.display = 'none'; document.getElementById('1104.4841v1-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> 26 April, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett., 106 145001, (2011) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1104.4661">arXiv:1104.4661</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1104.4661">pdf</a>, <a href="https://arxiv.org/ps/1104.4661">ps</a>, <a href="https://arxiv.org/format/1104.4661">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</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> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-ph</span> </div> </div> <p class="title is-5 mathjax"> Alpha Antihydrogen Experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=ALPHA+Collaboration"> ALPHA Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">G. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Bray%2C+C+C">C. C. Bray</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">S. Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">R. S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">A. J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">R. Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">L. Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Lambo%2C+R">R. Lambo</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a> , et al. (16 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="1104.4661v1-abstract-short" style="display: inline;"> ALPHA is an experiment at CERN, whose ultimate goal is to perform a precise test of CPT symmetry with trapped antihydrogen atoms. After reviewing the motivations, we discuss our recent progress toward the initial goal of stable trapping of antihydrogen, with some emphasis on particle detection techniques. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1104.4661v1-abstract-full" style="display: none;"> ALPHA is an experiment at CERN, whose ultimate goal is to perform a precise test of CPT symmetry with trapped antihydrogen atoms. After reviewing the motivations, we discuss our recent progress toward the initial goal of stable trapping of antihydrogen, with some emphasis on particle detection techniques. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1104.4661v1-abstract-full').style.display = 'none'; document.getElementById('1104.4661v1-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> 24 April, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2011. </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">Invited talk presented at the Fifth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 28-July 2, 2010</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Proceedings of the Fifth Meeting on CPT and Lorentz Symmetry, Ed. V.A. Kostelecky, pp. 50-54, World Scientific (2011) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1101.0808">arXiv:1101.0808</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1101.0808">pdf</a>, <a href="https://arxiv.org/format/1101.0808">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Statistical Mechanics">cond-mat.stat-mech</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="Biological Physics">physics.bio-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/PhysRevE.83.020102">10.1103/PhysRevE.83.020102 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental measurement of efficiency and transport coherence of a cold atom Brownian motor in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Zelan%2C+M">M. Zelan</a>, <a href="/search/physics?searchtype=author&amp;query=Hagman%2C+H">H. Hagman</a>, <a href="/search/physics?searchtype=author&amp;query=Labaigt%2C+G">G. Labaigt</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">C. M. Dion</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="1101.0808v2-abstract-short" style="display: inline;"> The rectification of noise into directed movement or useful energy is utilized by many different systems. The peculiar nature of the energy source and conceptual differences between such Brownian motor systems makes a characterization of the performance far from straightforward. In this work, where the Brownian motor consists of atoms interacting with dissipative optical lattices, we adopt existin&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1101.0808v2-abstract-full').style.display = 'inline'; document.getElementById('1101.0808v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1101.0808v2-abstract-full" style="display: none;"> The rectification of noise into directed movement or useful energy is utilized by many different systems. The peculiar nature of the energy source and conceptual differences between such Brownian motor systems makes a characterization of the performance far from straightforward. In this work, where the Brownian motor consists of atoms interacting with dissipative optical lattices, we adopt existing theory and present experimental measurements for both the efficiency and the transport coherence. We achieve up to 0.3% for the efficiency and 0.01 for the P茅clet number. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1101.0808v2-abstract-full').style.display = 'none'; document.getElementById('1101.0808v2-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> 25 January, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 January, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. E 83, 020102(R) (2011) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1012.4110">arXiv:1012.4110</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1012.4110">pdf</a>, <a href="https://arxiv.org/ps/1012.4110">ps</a>, <a href="https://arxiv.org/format/1012.4110">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="High Energy Physics - Experiment">hep-ex</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/10.1016/j.physletb.2010.11.004">10.1016/j.physletb.2010.11.004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search For Trapped Antihydrogen </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">Gorm B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">Mohammad D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">Marcelo Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">William Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Bowe%2C+P+D">Paul D. Bowe</a>, <a href="/search/physics?searchtype=author&amp;query=Bray%2C+C+C">Crystal C. Bray</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">Eoin Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">Claudio L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">Steven Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">Michael Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">Joel Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">Tim Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">Makoto C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">David R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">Jeffrey S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">Walter N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">Ryugo S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">Michael E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A+J">Andrew J. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">Richard Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=J%C3%B8rgensen%2C+L+V">Lars V. J酶rgensen</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">Lenoid Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Lambo%2C+R">Ricardo Lambo</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">Niels Madsen</a> , et al. (17 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="1012.4110v1-abstract-short" style="display: inline;"> We present the results of an experiment to search for trapped antihydrogen atoms with the ALPHA antihydrogen trap at the CERN Antiproton Decelerator. Sensitive diagnostics of the temperatures, sizes, and densities of the trapped antiproton and positron plasmas have been developed, which in turn permitted development of techniques to precisely and reproducibly control the initial experimental param&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1012.4110v1-abstract-full').style.display = 'inline'; document.getElementById('1012.4110v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1012.4110v1-abstract-full" style="display: none;"> We present the results of an experiment to search for trapped antihydrogen atoms with the ALPHA antihydrogen trap at the CERN Antiproton Decelerator. Sensitive diagnostics of the temperatures, sizes, and densities of the trapped antiproton and positron plasmas have been developed, which in turn permitted development of techniques to precisely and reproducibly control the initial experimental parameters. The use of a position-sensitive annihilation vertex detector, together with the capability of controllably quenching the superconducting magnetic minimum trap, enabled us to carry out a high-sensitivity and low-background search for trapped synthesised antihydrogen atoms. We aim to identify the annihilations of antihydrogen atoms held for at least 130 ms in the trap before being released over ~30 ms. After a three-week experimental run in 2009 involving mixing of 10^7 antiprotons with 1.3 10^9 positrons to produce 6 10^5 antihydrogen atoms, we have identified six antiproton annihilation events that are consistent with the release of trapped antihydrogen. The cosmic ray background, estimated to contribute 0.14 counts, is incompatible with this observation at a significance of 5.6 sigma. Extensive simulations predict that an alternative source of annihilations, the escape of mirror-trapped antiprotons, is highly unlikely, though this possibility has not yet been ruled out experimentally. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1012.4110v1-abstract-full').style.display = 'none'; document.getElementById('1012.4110v1-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> 18 December, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2010. </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">12 pages, 7 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physics Letters B 695 (2011) 95-104 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1009.4687">arXiv:1009.4687</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1009.4687">pdf</a>, <a href="https://arxiv.org/format/1009.4687">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Plasma Physics">physics.plasm-ph</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 Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-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/10.1103/PhysRevLett.105.013003">10.1103/PhysRevLett.105.013003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Evaporative Cooling of Antiprotons to Cryogenic Temperatures </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=ALPHA+Collaboration"> ALPHA Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Andresen%2C+G+B">G. B. Andresen</a>, <a href="/search/physics?searchtype=author&amp;query=Ashkezari%2C+M+D">M. D. Ashkezari</a>, <a href="/search/physics?searchtype=author&amp;query=Baquero-Ruiz%2C+M">M. Baquero-Ruiz</a>, <a href="/search/physics?searchtype=author&amp;query=Bertsche%2C+W">W. Bertsche</a>, <a href="/search/physics?searchtype=author&amp;query=Bowe%2C+P+D">P. D. Bowe</a>, <a href="/search/physics?searchtype=author&amp;query=Butler%2C+E">E. Butler</a>, <a href="/search/physics?searchtype=author&amp;query=Cesar%2C+C+L">C. L. Cesar</a>, <a href="/search/physics?searchtype=author&amp;query=Chapman%2C+S">S. Chapman</a>, <a href="/search/physics?searchtype=author&amp;query=Charlton%2C+M">M. Charlton</a>, <a href="/search/physics?searchtype=author&amp;query=Fajans%2C+J">J. Fajans</a>, <a href="/search/physics?searchtype=author&amp;query=Friesen%2C+T">T. Friesen</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+M+C">M. C. Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Gill%2C+D+R">D. R. Gill</a>, <a href="/search/physics?searchtype=author&amp;query=Hangst%2C+J+S">J. S. Hangst</a>, <a href="/search/physics?searchtype=author&amp;query=Hardy%2C+W+N">W. N. Hardy</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">R. S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hayden%2C+M+E">M. E. Hayden</a>, <a href="/search/physics?searchtype=author&amp;query=Humphries%2C+A">A. Humphries</a>, <a href="/search/physics?searchtype=author&amp;query=Hydomako%2C+R">R. Hydomako</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kurchaninov%2C+L">L. Kurchaninov</a>, <a href="/search/physics?searchtype=author&amp;query=Lambo%2C+R">R. Lambo</a>, <a href="/search/physics?searchtype=author&amp;query=Madsen%2C+N">N. Madsen</a>, <a href="/search/physics?searchtype=author&amp;query=Menary%2C+S">S. Menary</a> , et al. (15 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="1009.4687v1-abstract-short" style="display: inline;"> We report the application of evaporative cooling to clouds of trapped antiprotons, resulting in plasmas with measured temperature as low as 9~K. We have modeled the evaporation process for charged particles using appropriate rate equations. Good agreement between experiment and theory is observed, permitting prediction of cooling efficiency in future experiments. The technique opens up new possibi&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.4687v1-abstract-full').style.display = 'inline'; document.getElementById('1009.4687v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1009.4687v1-abstract-full" style="display: none;"> We report the application of evaporative cooling to clouds of trapped antiprotons, resulting in plasmas with measured temperature as low as 9~K. We have modeled the evaporation process for charged particles using appropriate rate equations. Good agreement between experiment and theory is observed, permitting prediction of cooling efficiency in future experiments. The technique opens up new possibilities for cooling of trapped ions and is of particular interest in antiproton physics, where a precise \emph{CPT} test on trapped antihydrogen is a long-standing goal. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.4687v1-abstract-full').style.display = 'none'; document.getElementById('1009.4687v1-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> 23 September, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2010. </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">5 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.105:013003,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0803.2153">arXiv:0803.2153</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0803.2153">pdf</a>, <a href="https://arxiv.org/ps/0803.2153">ps</a>, <a href="https://arxiv.org/format/0803.2153">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> </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/epjd/e2008-00080-8">10.1140/epjd/e2008-00080-8 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Simulations of Sisyphus cooling including multiple excited states </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Svensson%2C+F">F. Svensson</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">C. M. Dion</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="0803.2153v1-abstract-short" style="display: inline;"> We extend the theory for laser cooling in a near-resonant optical lattice to include multiple excited hyperfine states. Simulations are performed treating the external degrees of freedom of the atom, i.e., position and momentum, classically, while the internal atomic states are treated quantum mechanically, allowing for arbitrary superpositions. Whereas theoretical treatments including only a si&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0803.2153v1-abstract-full').style.display = 'inline'; document.getElementById('0803.2153v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0803.2153v1-abstract-full" style="display: none;"> We extend the theory for laser cooling in a near-resonant optical lattice to include multiple excited hyperfine states. Simulations are performed treating the external degrees of freedom of the atom, i.e., position and momentum, classically, while the internal atomic states are treated quantum mechanically, allowing for arbitrary superpositions. Whereas theoretical treatments including only a single excited hyperfine state predict that the temperature should be a function of lattice depth only, except close to resonance, experiments have shown that the minimum temperature achieved depends also on the detuning from resonance of the lattice light. Our results resolve this discrepancy. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0803.2153v1-abstract-full').style.display = 'none'; document.getElementById('0803.2153v1-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> 14 March, 2008; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2008. </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">7 pages, 6 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0704.3955">arXiv:0704.3955</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0704.3955">pdf</a>, <a href="https://arxiv.org/format/0704.3955">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> </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/epjd/e2007-00233-3">10.1140/epjd/e2007-00233-3 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Characterisation of a three-dimensional Brownian motor in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Sjolund%2C+P">P. Sjolund</a>, <a href="/search/physics?searchtype=author&amp;query=Petra%2C+S+J+H">S. J. H. Petra</a>, <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">C. M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Hagman%2C+H">H. Hagman</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">A. Kastberg</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="0704.3955v1-abstract-short" style="display: inline;"> We present here a detailed study of the behaviour of a three dimensional Brownian motor based on cold atoms in a double optical lattice [P. Sjolund et al., Phys. Rev. Lett. 96, 190602 (2006)]. This includes both experiments and numerical simulations of a Brownian particle. The potentials used are spatially and temporally symmetric, but combined spatiotemporal symmetry is broken by phase shifts a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0704.3955v1-abstract-full').style.display = 'inline'; document.getElementById('0704.3955v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0704.3955v1-abstract-full" style="display: none;"> We present here a detailed study of the behaviour of a three dimensional Brownian motor based on cold atoms in a double optical lattice [P. Sjolund et al., Phys. Rev. Lett. 96, 190602 (2006)]. This includes both experiments and numerical simulations of a Brownian particle. The potentials used are spatially and temporally symmetric, but combined spatiotemporal symmetry is broken by phase shifts and asymmetric transfer rates between potentials. The diffusion of atoms in the optical lattices is rectified and controlled both in direction and speed along three dimensions. We explore a large range of experimental parameters, where irradiances and detunings of the optical lattice lights are varied within the dissipative regime. Induced drift velocities in the order of one atomic recoil velocity have been achieved. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0704.3955v1-abstract-full').style.display = 'none'; document.getElementById('0704.3955v1-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> 30 April, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2007. </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">8 pages, 14 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. D 44, 381 (2007) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0611302">arXiv:physics/0611302</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0611302">pdf</a>, <a href="https://arxiv.org/ps/physics/0611302">ps</a>, <a href="https://arxiv.org/format/physics/0611302">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> </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/epjst/e2008-00688-8">10.1140/epjst/e2008-00688-8 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Controllable 3D atomic Brownian motor in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">Claude M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Sjolund%2C+P">Peder Sjolund</a>, <a href="/search/physics?searchtype=author&amp;query=Petra%2C+S+J+H">Stefan J. H. Petra</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Nylen%2C+M">Mats Nylen</a>, <a href="/search/physics?searchtype=author&amp;query=Sanchez-Palencia%2C+L">Laurent Sanchez-Palencia</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">Anders Kastberg</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/0611302v1-abstract-short" style="display: inline;"> We study a Brownian motor, based on cold atoms in optical lattices, where atomic motion can be induced in a controlled manner in an arbitrary direction, by rectification of isotropic random fluctuations. In contrast with ratchet mechanisms, our Brownian motor operates in a potential that is spatially and temporally symmetric, in apparent contradiction to the Curie principle. Simulations, based o&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0611302v1-abstract-full').style.display = 'inline'; document.getElementById('physics/0611302v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0611302v1-abstract-full" style="display: none;"> We study a Brownian motor, based on cold atoms in optical lattices, where atomic motion can be induced in a controlled manner in an arbitrary direction, by rectification of isotropic random fluctuations. In contrast with ratchet mechanisms, our Brownian motor operates in a potential that is spatially and temporally symmetric, in apparent contradiction to the Curie principle. Simulations, based on the Fokker-Planck equation, allow us to gain knowledge on the qualitative behaviour of our Brownian motor. Studies of Brownian motors, and in particular ones with unique control properties, are of fundamental interest because of the role they play in protein motors and their potential applications in nanotechnology. In particular, our system opens the way to the study of quantum Brownian motors. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0611302v1-abstract-full').style.display = 'none'; document.getElementById('physics/0611302v1-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> 30 November, 2006; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2006. </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">7 pages, 4 figures. Presented at the conference &#34;Theoretical and Experimental Foundations of Recent Quantum Technologies&#34; (Durban, South Africa)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. Special Topics 159, 11 (2008) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0512188">arXiv:physics/0512188</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0512188">pdf</a>, <a href="https://arxiv.org/ps/physics/0512188">ps</a>, <a href="https://arxiv.org/format/physics/0512188">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> </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/10.1016/j.nimb.2006.01.050">10.1016/j.nimb.2006.01.050 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Low-temperature antihydrogen-atom scattering </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S Jonsell</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/0512188v1-abstract-short" style="display: inline;"> A simple method to include the strong force in atom-antiatom scattering is presented. It is based on the strong-force scatteringn length between the nucleon and antinucleon. Using this method elastic and annihilation cross sections are calculated for hydrogen-antihydrogen and helium-antihydrogen scattering. The results are compared to first-order perturbation theory using a pseudo potential. The&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512188v1-abstract-full').style.display = 'inline'; document.getElementById('physics/0512188v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0512188v1-abstract-full" style="display: none;"> A simple method to include the strong force in atom-antiatom scattering is presented. It is based on the strong-force scatteringn length between the nucleon and antinucleon. Using this method elastic and annihilation cross sections are calculated for hydrogen-antihydrogen and helium-antihydrogen scattering. The results are compared to first-order perturbation theory using a pseudo potential. The pseudo-potential approach works fairly well for hydrogen-antihydrogen scattering, but fails for helium-antihydrogen scattering where strong-force effects are more prominent. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512188v1-abstract-full').style.display = 'none'; document.getElementById('physics/0512188v1-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> 20 December, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2005. </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">9 pages, 2 figures, to be published in Nuclear Instruments and Methods B</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0512159">arXiv:physics/0512159</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0512159">pdf</a>, <a href="https://arxiv.org/ps/physics/0512159">ps</a>, <a href="https://arxiv.org/format/physics/0512159">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> </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/epjd/e2006-00082-6">10.1140/epjd/e2006-00082-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A nonadiabatic semi-classical method for dynamics of atoms in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">S. Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">C. M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Nyl%C3%A9n%2C+M">M. Nyl茅n</a>, <a href="/search/physics?searchtype=author&amp;query=Petra%2C+S+J+H">S. J. H. Petra</a>, <a href="/search/physics?searchtype=author&amp;query=Sj%C3%B6lund%2C+P">P. Sj枚lund</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">A. Kastberg</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/0512159v1-abstract-short" style="display: inline;"> We develop a semi-classical method to simulate the motion of atoms in a dissipative optical lattice. Our method treats the internal states of the atom quantum mechanically, including all nonadiabatic couplings, while position and momentum are treated as classical variables. We test our method in the one-dimensional case. Excellent agreement with fully quantum mechanical simulations is found. Our&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512159v1-abstract-full').style.display = 'inline'; document.getElementById('physics/0512159v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0512159v1-abstract-full" style="display: none;"> We develop a semi-classical method to simulate the motion of atoms in a dissipative optical lattice. Our method treats the internal states of the atom quantum mechanically, including all nonadiabatic couplings, while position and momentum are treated as classical variables. We test our method in the one-dimensional case. Excellent agreement with fully quantum mechanical simulations is found. Our results are much more accurate than those of earlier semi-classical methods based on the adiabatic approximation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512159v1-abstract-full').style.display = 'none'; document.getElementById('physics/0512159v1-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> 16 December, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2005. </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">7 pages, 5 figures, submitted to European Physical Journal D</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0512145">arXiv:physics/0512145</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0512145">pdf</a>, <a href="https://arxiv.org/ps/physics/0512145">ps</a>, <a href="https://arxiv.org/format/physics/0512145">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> </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.96.190602">10.1103/PhysRevLett.96.190602 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Demonstration of a controllable three-dimensional Brownian motor in symmetric potentials </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Sjolund%2C+P">Peder Sjolund</a>, <a href="/search/physics?searchtype=author&amp;query=Petra%2C+S+J+H">Stefan J. H. Petra</a>, <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">Claude M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Nylen%2C+M">Mats Nylen</a>, <a href="/search/physics?searchtype=author&amp;query=Sanchez-Palencia%2C+L">Laurent Sanchez-Palencia</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">Anders Kastberg</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/0512145v2-abstract-short" style="display: inline;"> We demonstrate a Brownian motor, based on cold atoms in optical lattices, where isotropic random fluctuations are rectified in order to induce controlled atomic motion in arbitrary directions. In contrast to earlier demonstrations of ratchet effects, our Brownian motor operates in potentials that are spatially and temporally symmetric, but where spatiotemporal symmetry is broken by a phase shift&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512145v2-abstract-full').style.display = 'inline'; document.getElementById('physics/0512145v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0512145v2-abstract-full" style="display: none;"> We demonstrate a Brownian motor, based on cold atoms in optical lattices, where isotropic random fluctuations are rectified in order to induce controlled atomic motion in arbitrary directions. In contrast to earlier demonstrations of ratchet effects, our Brownian motor operates in potentials that are spatially and temporally symmetric, but where spatiotemporal symmetry is broken by a phase shift between the potentials and asymmetric transfer rates between them. The Brownian motor is demonstrated in three dimensions and the noise-induced drift is controllable in our system. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0512145v2-abstract-full').style.display = 'none'; document.getElementById('physics/0512145v2-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> 24 April, 2006; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 December, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2005. </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">5 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 96, 190602 (2006) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/0506119">arXiv:physics/0506119</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/0506119">pdf</a>, <a href="https://arxiv.org/ps/physics/0506119">ps</a>, <a href="https://arxiv.org/format/physics/0506119">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="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/10.1209/epl/i2005-10244-6">10.1209/epl/i2005-10244-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Time dependence of laser cooling in optical lattices </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Dion%2C+C+M">Claude M. Dion</a>, <a href="/search/physics?searchtype=author&amp;query=Sjolund%2C+P">Peder Sjolund</a>, <a href="/search/physics?searchtype=author&amp;query=Petra%2C+S+J+H">Stefan J. H. Petra</a>, <a href="/search/physics?searchtype=author&amp;query=Jonsell%2C+S">Svante Jonsell</a>, <a href="/search/physics?searchtype=author&amp;query=Kastberg%2C+A">Anders Kastberg</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/0506119v2-abstract-short" style="display: inline;"> We study the dynamics of the cooling of a gas of caesium atoms in an optical lattice, both experimentally and with 1D full-quantum Monte Carlo simulations. We find that, contrary to the standard interpretation of the Sisyphus model, the cooling process does not work by a continuous decrease of the average kinetic energy of the atoms in the lattice. Instead, we show that the momentum of the atoms&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0506119v2-abstract-full').style.display = 'inline'; document.getElementById('physics/0506119v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/0506119v2-abstract-full" style="display: none;"> We study the dynamics of the cooling of a gas of caesium atoms in an optical lattice, both experimentally and with 1D full-quantum Monte Carlo simulations. We find that, contrary to the standard interpretation of the Sisyphus model, the cooling process does not work by a continuous decrease of the average kinetic energy of the atoms in the lattice. Instead, we show that the momentum of the atoms follows a bimodal distribution, the atoms being gradually transferred from a hot to a cold mode. We suggest that the cooling mechanism should be depicted in terms of a rate model, describing the transfer between the two modes along with the processes occurring within each mode. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/0506119v2-abstract-full').style.display = 'none'; document.getElementById('physics/0506119v2-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> 5 September, 2005; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 June, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2005. </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">7 pages, 5 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Europhys. Lett., 72 (3), pp. 369-375 (2005) </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="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div> <!-- end MetaColumn 1 --> <!-- MetaColumn 2 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div> <!-- end MetaColumn 2 --> </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

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