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is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</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.123.111101">10.1103/PhysRevLett.123.111101 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Armano%2C+M">M. Armano</a>, <a href="/search/physics?searchtype=author&amp;query=Audley%2C+H">H. Audley</a>, <a href="/search/physics?searchtype=author&amp;query=Baird%2C+J">J. Baird</a>, <a href="/search/physics?searchtype=author&amp;query=Binetruy%2C+P">P. Binetruy</a>, <a href="/search/physics?searchtype=author&amp;query=Born%2C+M">M. Born</a>, <a href="/search/physics?searchtype=author&amp;query=Bortoluzzi%2C+D">D. Bortoluzzi</a>, <a href="/search/physics?searchtype=author&amp;query=Castelli%2C+E">E. Castelli</a>, <a href="/search/physics?searchtype=author&amp;query=Cavalleri%2C+A">A. Cavalleri</a>, <a href="/search/physics?searchtype=author&amp;query=Cesarini%2C+A">A. Cesarini</a>, <a href="/search/physics?searchtype=author&amp;query=Cruise%2C+A+M">A. M. Cruise</a>, <a href="/search/physics?searchtype=author&amp;query=Danzmann%2C+K">K. Danzmann</a>, <a href="/search/physics?searchtype=author&amp;query=Silva%2C+M+d+D">M. de Deus Silva</a>, <a href="/search/physics?searchtype=author&amp;query=Diepholz%2C+I">I. Diepholz</a>, <a href="/search/physics?searchtype=author&amp;query=Dixon%2C+G">G. Dixon</a>, <a href="/search/physics?searchtype=author&amp;query=Dolesi%2C+R">R. Dolesi</a>, <a href="/search/physics?searchtype=author&amp;query=Ferraioli%2C+L">L. Ferraioli</a>, <a href="/search/physics?searchtype=author&amp;query=Ferroni%2C+V">V. Ferroni</a>, <a href="/search/physics?searchtype=author&amp;query=Fitzsimons%2C+E+D">E. D. Fitzsimons</a>, <a href="/search/physics?searchtype=author&amp;query=Freschi%2C+M">M. Freschi</a>, <a href="/search/physics?searchtype=author&amp;query=Gesa%2C+L">L. Gesa</a>, <a href="/search/physics?searchtype=author&amp;query=Gibert%2C+F">F. Gibert</a>, <a href="/search/physics?searchtype=author&amp;query=Giardini%2C+D">D. Giardini</a>, <a href="/search/physics?searchtype=author&amp;query=Giusteri%2C+R">R. Giusteri</a>, <a href="/search/physics?searchtype=author&amp;query=Grimani%2C+C">C. Grimani</a>, <a href="/search/physics?searchtype=author&amp;query=Grzymisch%2C+J">J. Grzymisch</a> , et al. (53 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="1908.11584v1-abstract-short" style="display: inline;"> We report on the results of the LISA Pathfinder (LPF) free-fall mode experiment, in which the control force needed to compensate the quasistatic differential force acting on two test masses is applied intermittently as a series of &#34;impulse&#34; forces lasting a few seconds and separated by roughly 350 s periods of true free fall. This represents an alternative to the normal LPF mode of operation in wh&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1908.11584v1-abstract-full').style.display = 'inline'; document.getElementById('1908.11584v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1908.11584v1-abstract-full" style="display: none;"> We report on the results of the LISA Pathfinder (LPF) free-fall mode experiment, in which the control force needed to compensate the quasistatic differential force acting on two test masses is applied intermittently as a series of &#34;impulse&#34; forces lasting a few seconds and separated by roughly 350 s periods of true free fall. This represents an alternative to the normal LPF mode of operation in which this balancing force is applied continuously, with the advantage that the acceleration noise during free fall is measured in the absence of the actuation force, thus eliminating associated noise and force calibration errors. The differential acceleration noise measurement presented here with the free-fall mode agrees with noise measured with the continuous actuation scheme, representing an important and independent confirmation of the LPF result. An additional measurement with larger actuation forces also shows that the technique can be used to eliminate actuation noise when this is a dominant factor. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1908.11584v1-abstract-full').style.display = 'none'; document.getElementById('1908.11584v1-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, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2019. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1904.04694">arXiv:1904.04694</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1904.04694">pdf</a>, <a href="https://arxiv.org/ps/1904.04694">ps</a>, <a href="https://arxiv.org/format/1904.04694">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Space Physics">physics.space-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Earth and Planetary Astrophysics">astro-ph.EP</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</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/10.3847/1538-4357/ab0c99">10.3847/1538-4357/ab0c99 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Forbush decreases and $&lt;$ 2-day GCR flux non-recurrent variations studied with LISA Pathfinder </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Grimani%2C+C">C. Grimani</a>, <a href="/search/physics?searchtype=author&amp;query=Armano%2C+M">M. Armano</a>, <a href="/search/physics?searchtype=author&amp;query=Audley%2C+H">H. Audley</a>, <a href="/search/physics?searchtype=author&amp;query=Baird%2C+J">J. Baird</a>, <a href="/search/physics?searchtype=author&amp;query=Benella%2C+S">S. Benella</a>, <a href="/search/physics?searchtype=author&amp;query=Binetruy%2C+P">P. Binetruy</a>, <a href="/search/physics?searchtype=author&amp;query=Born%2C+M">M. Born</a>, <a href="/search/physics?searchtype=author&amp;query=Bortoluzzi%2C+D">D. Bortoluzzi</a>, <a href="/search/physics?searchtype=author&amp;query=Castelli%2C+E">E. Castelli</a>, <a href="/search/physics?searchtype=author&amp;query=Cavalleri%2C+A">A. Cavalleri</a>, <a href="/search/physics?searchtype=author&amp;query=Cesarini%2C+A">A. Cesarini</a>, <a href="/search/physics?searchtype=author&amp;query=Cruise%2C+A+M">A. M. Cruise</a>, <a href="/search/physics?searchtype=author&amp;query=Danzmann%2C+K">K. Danzmann</a>, <a href="/search/physics?searchtype=author&amp;query=Silva%2C+M+d+D">M. de Deus Silva</a>, <a href="/search/physics?searchtype=author&amp;query=Diepholz%2C+I">I. Diepholz</a>, <a href="/search/physics?searchtype=author&amp;query=Dixon%2C+G">G. Dixon</a>, <a href="/search/physics?searchtype=author&amp;query=Dolesi%2C+R">R. Dolesi</a>, <a href="/search/physics?searchtype=author&amp;query=Fabi%2C+M">M. Fabi</a>, <a href="/search/physics?searchtype=author&amp;query=Ferraioli%2C+L">L. Ferraioli</a>, <a href="/search/physics?searchtype=author&amp;query=Ferroni%2C+V">V. Ferroni</a>, <a href="/search/physics?searchtype=author&amp;query=Finetti%2C+N">N. Finetti</a>, <a href="/search/physics?searchtype=author&amp;query=Fitzsimons%2C+E+D">E. D. Fitzsimons</a>, <a href="/search/physics?searchtype=author&amp;query=Freschi%2C+M">M. Freschi</a>, <a href="/search/physics?searchtype=author&amp;query=Gesa%2C+L">L. Gesa</a>, <a href="/search/physics?searchtype=author&amp;query=Gibert%2C+F">F. Gibert</a> , et al. (60 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="1904.04694v1-abstract-short" style="display: inline;"> Non-recurrent short term variations of the galactic cosmic-ray (GCR) flux above 70 MeV n$^{-1}$ were observed between 2016 February 18 and 2017 July 3 aboard the European Space Agency LISA Pathfinder (LPF) mission orbiting around the Lagrange point L1 at 1.5$\times$10$^6$ km from Earth. The energy dependence of three Forbush decreases (FDs) is studied and reported here. A comparison of these obser&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1904.04694v1-abstract-full').style.display = 'inline'; document.getElementById('1904.04694v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1904.04694v1-abstract-full" style="display: none;"> Non-recurrent short term variations of the galactic cosmic-ray (GCR) flux above 70 MeV n$^{-1}$ were observed between 2016 February 18 and 2017 July 3 aboard the European Space Agency LISA Pathfinder (LPF) mission orbiting around the Lagrange point L1 at 1.5$\times$10$^6$ km from Earth. The energy dependence of three Forbush decreases (FDs) is studied and reported here. A comparison of these observations with others carried out in space down to the energy of a few tens of MeV n$^{-1}$ shows that the same GCR flux parameterization applies to events of different intensity during the main phase. FD observations in L1 with LPF and geomagnetic storm occurrence is also presented. Finally, the characteristics of GCR flux non-recurrent variations (peaks and depressions) of duration $&lt;$ 2 days and their association with interplanetary structures are investigated. It is found that, most likely, plasma compression regions between subsequent corotating high-speed streams cause peaks, while heliospheric current sheet crossing cause the majority of the depressions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1904.04694v1-abstract-full').style.display = 'none'; document.getElementById('1904.04694v1-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 April, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> M. Armano et al 2019 ApJ 874 167 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.02435">arXiv:1807.02435</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.02435">pdf</a>, <a href="https://arxiv.org/format/1807.02435">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/10.1103/PhysRevD.98.062001">10.1103/PhysRevD.98.062001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Precision Charge Control for Isolated Free-Falling Test Masses: LISA Pathfinder Results </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Armano%2C+M">M. Armano</a>, <a href="/search/physics?searchtype=author&amp;query=Audley%2C+H">H. Audley</a>, <a href="/search/physics?searchtype=author&amp;query=Baird%2C+J">J. Baird</a>, <a href="/search/physics?searchtype=author&amp;query=Binetruy%2C+P">P. Binetruy</a>, <a href="/search/physics?searchtype=author&amp;query=Born%2C+M">M. Born</a>, <a href="/search/physics?searchtype=author&amp;query=Bortoluzzi%2C+D">D. Bortoluzzi</a>, <a href="/search/physics?searchtype=author&amp;query=Castelli%2C+E">E. Castelli</a>, <a href="/search/physics?searchtype=author&amp;query=Cavalleri%2C+A">A. Cavalleri</a>, <a href="/search/physics?searchtype=author&amp;query=Cesarini%2C+A">A. Cesarini</a>, <a href="/search/physics?searchtype=author&amp;query=Cruise%2C+A+M">A. M. Cruise</a>, <a href="/search/physics?searchtype=author&amp;query=Danzmann%2C+K">K. Danzmann</a>, <a href="/search/physics?searchtype=author&amp;query=Silva%2C+M+d+D">M. de Deus Silva</a>, <a href="/search/physics?searchtype=author&amp;query=Diepholz%2C+I">I. Diepholz</a>, <a href="/search/physics?searchtype=author&amp;query=Dixon%2C+G">G. Dixon</a>, <a href="/search/physics?searchtype=author&amp;query=Dolesi%2C+R">R. Dolesi</a>, <a href="/search/physics?searchtype=author&amp;query=Ferraioli%2C+L">L. Ferraioli</a>, <a href="/search/physics?searchtype=author&amp;query=Ferroni%2C+V">V. Ferroni</a>, <a href="/search/physics?searchtype=author&amp;query=Fitzsimons%2C+E+D">E. D. Fitzsimons</a>, <a href="/search/physics?searchtype=author&amp;query=Freschi%2C+M">M. Freschi</a>, <a href="/search/physics?searchtype=author&amp;query=Gesa%2C+L">L. Gesa</a>, <a href="/search/physics?searchtype=author&amp;query=Giardini%2C+D">D. Giardini</a>, <a href="/search/physics?searchtype=author&amp;query=Gibert%2C+F">F. Gibert</a>, <a href="/search/physics?searchtype=author&amp;query=Giusteri%2C+R">R. Giusteri</a>, <a href="/search/physics?searchtype=author&amp;query=Grimani%2C+C">C. Grimani</a>, <a href="/search/physics?searchtype=author&amp;query=Grzymisch%2C+J">J. Grzymisch</a> , et al. (60 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="1807.02435v2-abstract-short" style="display: inline;"> The LISA Pathfinder charge management device was responsible for neutralising the cosmic ray induced electric charge that inevitably accumulated on the free-falling test masses at the heart of the experiment. We present measurements made on ground and in-flight that quantify the performance of this contactless discharge system which was based on photo-emission under UV illumination. In addition, a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.02435v2-abstract-full').style.display = 'inline'; document.getElementById('1807.02435v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.02435v2-abstract-full" style="display: none;"> The LISA Pathfinder charge management device was responsible for neutralising the cosmic ray induced electric charge that inevitably accumulated on the free-falling test masses at the heart of the experiment. We present measurements made on ground and in-flight that quantify the performance of this contactless discharge system which was based on photo-emission under UV illumination. In addition, a two-part simulation is described that was developed alongside the hardware. Modelling of the absorbed UV light within the Pathfinder sensor was carried out with the GEANT4 software toolkit and a separate MATLAB charge transfer model calculated the net photocurrent between the test masses and surrounding housing in the presence of AC and DC electric fields. We confront the results of these models with observations and draw conclusions for the design of discharge systems for future experiments like LISA that will also employ free-falling test masses. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.02435v2-abstract-full').style.display = 'none'; document.getElementById('1807.02435v2-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> 17 September, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 98, 062001 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1802.09374">arXiv:1802.09374</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1802.09374">pdf</a>, <a href="https://arxiv.org/ps/1802.09374">ps</a>, <a href="https://arxiv.org/format/1802.09374">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Space Physics">physics.space-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</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/10.3847/1538-4357/aaa774">10.3847/1538-4357/aaa774 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a Forbush decrease with LISA Pathfinder </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Armano%2C+M">M. Armano</a>, <a href="/search/physics?searchtype=author&amp;query=Audley%2C+H">H. Audley</a>, <a href="/search/physics?searchtype=author&amp;query=Baird%2C+J">J. Baird</a>, <a href="/search/physics?searchtype=author&amp;query=Bassan%2C+M">M. Bassan</a>, <a href="/search/physics?searchtype=author&amp;query=Benella%2C+S">S. Benella</a>, <a href="/search/physics?searchtype=author&amp;query=Binetruy%2C+P">P. Binetruy</a>, <a href="/search/physics?searchtype=author&amp;query=Born%2C+M">M. Born</a>, <a href="/search/physics?searchtype=author&amp;query=Bortoluzzi%2C+D">D. Bortoluzzi</a>, <a href="/search/physics?searchtype=author&amp;query=Cavalleri%2C+A">A. Cavalleri</a>, <a href="/search/physics?searchtype=author&amp;query=Cesarini%2C+A">A. Cesarini</a>, <a href="/search/physics?searchtype=author&amp;query=Cruise%2C+A+M">A. M. Cruise</a>, <a href="/search/physics?searchtype=author&amp;query=Danzmann%2C+K">K. Danzmann</a>, <a href="/search/physics?searchtype=author&amp;query=Silva%2C+M+d+D">M. de Deus Silva</a>, <a href="/search/physics?searchtype=author&amp;query=Diepholz%2C+I">I. Diepholz</a>, <a href="/search/physics?searchtype=author&amp;query=Dixon%2C+G">G. Dixon</a>, <a href="/search/physics?searchtype=author&amp;query=Dolesi%2C+R">R. Dolesi</a>, <a href="/search/physics?searchtype=author&amp;query=Fabi%2C+M">M. Fabi</a>, <a href="/search/physics?searchtype=author&amp;query=Ferraioli%2C+L">L. Ferraioli</a>, <a href="/search/physics?searchtype=author&amp;query=Ferroni%2C+V">V. Ferroni</a>, <a href="/search/physics?searchtype=author&amp;query=Finetti%2C+N">N. Finetti</a>, <a href="/search/physics?searchtype=author&amp;query=Fitzsimons%2C+E+D">E. D. Fitzsimons</a>, <a href="/search/physics?searchtype=author&amp;query=Freschi%2C+M">M. Freschi</a>, <a href="/search/physics?searchtype=author&amp;query=Gesa%2C+L">L. Gesa</a>, <a href="/search/physics?searchtype=author&amp;query=Gibert%2C+F">F. Gibert</a>, <a href="/search/physics?searchtype=author&amp;query=Giardini%2C+D">D. Giardini</a> , et al. (60 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="1802.09374v2-abstract-short" style="display: inline;"> Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high counting rate particle detector (PD) aboard LISA Pathfinder (LPF), meant for subsystems diagnostics, was devoted to the measurement of galactic cosmic-ray and solar energetic particle integral fluxes above 70 Me&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1802.09374v2-abstract-full').style.display = 'inline'; document.getElementById('1802.09374v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1802.09374v2-abstract-full" style="display: none;"> Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high counting rate particle detector (PD) aboard LISA Pathfinder (LPF), meant for subsystems diagnostics, was devoted to the measurement of galactic cosmic-ray and solar energetic particle integral fluxes above 70 MeV n$^{-1}$ up to 6500 counts s$^{-1}$. PD data were gathered with a sampling time of 15 s. Characteristics and energy-dependence of GCR flux recurrent depressions and of a Forbush decrease dated August 2, 2016 are reported here. The capability of interplanetary missions, carrying PDs for instrument performance purposes, in monitoring the passage of interplanetary coronal mass ejections (ICMEs) is also discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1802.09374v2-abstract-full').style.display = 'none'; document.getElementById('1802.09374v2-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> 27 April, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 23 February, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> The Astrophysical Journal, 854, 2018, 113 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1111.7252">arXiv:1111.7252</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1111.7252">pdf</a>, <a href="https://arxiv.org/format/1111.7252">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.1007/s00340-012-4878-z">10.1007/s00340-012-4878-z <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The 10m AEI prototype facility A brief overview </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Westphal%2C+T">Tobias Westphal</a>, <a href="/search/physics?searchtype=author&amp;query=Bergmann%2C+G">Gerald Bergmann</a>, <a href="/search/physics?searchtype=author&amp;query=Bertolini%2C+A">Alessandro Bertolini</a>, <a href="/search/physics?searchtype=author&amp;query=Born%2C+M">Michael Born</a>, <a href="/search/physics?searchtype=author&amp;query=Chen%2C+Y">Yanbei Chen</a>, <a href="/search/physics?searchtype=author&amp;query=Cumming%2C+A+V">Alan V Cumming</a>, <a href="/search/physics?searchtype=author&amp;query=Cunningham%2C+L">Liam Cunningham</a>, <a href="/search/physics?searchtype=author&amp;query=Dahl%2C+K">Katrin Dahl</a>, <a href="/search/physics?searchtype=author&amp;query=Graef%2C+C">Christian Graef</a>, <a href="/search/physics?searchtype=author&amp;query=Hammond%2C+G">Giles Hammond</a>, <a href="/search/physics?searchtype=author&amp;query=Heinzel%2C+G">Gerhard Heinzel</a>, <a href="/search/physics?searchtype=author&amp;query=Hild%2C+S">Stefan Hild</a>, <a href="/search/physics?searchtype=author&amp;query=Huttner%2C+S">Sabina Huttner</a>, <a href="/search/physics?searchtype=author&amp;query=Jones%2C+R">Russel Jones</a>, <a href="/search/physics?searchtype=author&amp;query=Kawazoe%2C+F">Fumiko Kawazoe</a>, <a href="/search/physics?searchtype=author&amp;query=Koehlenbeck%2C+S">Sina Koehlenbeck</a>, <a href="/search/physics?searchtype=author&amp;query=Kuehn%2C+G">Gerrit Kuehn</a>, <a href="/search/physics?searchtype=author&amp;query=Lueck%2C+H">Harald Lueck</a>, <a href="/search/physics?searchtype=author&amp;query=Mossavi%2C+K">Kasem Mossavi</a>, <a href="/search/physics?searchtype=author&amp;query=Poeld%2C+J+H">Jan H Poeld</a>, <a href="/search/physics?searchtype=author&amp;query=Somiya%2C+K">Kentaro Somiya</a>, <a href="/search/physics?searchtype=author&amp;query=van+Veggel%2C+M">Marielle van Veggel</a>, <a href="/search/physics?searchtype=author&amp;query=Wanner%2C+A">Alexander Wanner</a>, <a href="/search/physics?searchtype=author&amp;query=Willke%2C+B">Benno Willke</a>, <a href="/search/physics?searchtype=author&amp;query=Strain%2C+K+A">Ken A Strain</a> , et al. (2 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="1111.7252v2-abstract-short" style="display: inline;"> The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein Institute in Hannover, Germany. It aims to perform experiments for future gravitational wave detectors using advanced techniques. Seismically isolated benches are planned to be interferometrically interconnected and stabilized, forming a low-noise testbed inside a 100 m^3 ultra-high vacuum system.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.7252v2-abstract-full').style.display = 'inline'; document.getElementById('1111.7252v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1111.7252v2-abstract-full" style="display: none;"> The AEI 10 m prototype interferometer facility is currently being constructed at the Albert Einstein Institute in Hannover, Germany. It aims to perform experiments for future gravitational wave detectors using advanced techniques. Seismically isolated benches are planned to be interferometrically interconnected and stabilized, forming a low-noise testbed inside a 100 m^3 ultra-high vacuum system. A well-stabilized high power laser will perform differential position readout of 100 g test masses in a 10 m suspended arm-cavity enhanced Michelson interferometer at the crossover of measurement (shot) noise and backaction (quantum radiation pressure) noise, the so-called Standard Quantum Limit (SQL). Such a sensitivity enables experiments in the highly topical field of macroscopic quantum mechanics. In this article we introduce the experimental facility and describe the methods employed, technical details of subsystems will be covered in future papers. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.7252v2-abstract-full').style.display = 'none'; document.getElementById('1111.7252v2-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> 28 December, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 30 November, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2011. </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 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