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is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-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/10.1103/PhysRevAccelBeams.27.084802">10.1103/PhysRevAccelBeams.27.084802 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Continuous Electron Beam Accelerator Facility at 12 GeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adderley%2C+P+A">P. A. Adderley</a>, <a href="/search/physics?searchtype=author&amp;query=Ahmed%2C+S">S. Ahmed</a>, <a href="/search/physics?searchtype=author&amp;query=Allison%2C+T">T. Allison</a>, <a href="/search/physics?searchtype=author&amp;query=Bachimanchi%2C+R">R. Bachimanchi</a>, <a href="/search/physics?searchtype=author&amp;query=Baggett%2C+K">K. Baggett</a>, <a href="/search/physics?searchtype=author&amp;query=BastaniNejad%2C+M">M. BastaniNejad</a>, <a href="/search/physics?searchtype=author&amp;query=Bevins%2C+B">B. Bevins</a>, <a href="/search/physics?searchtype=author&amp;query=Bevins%2C+M">M. Bevins</a>, <a href="/search/physics?searchtype=author&amp;query=Bickley%2C+M">M. Bickley</a>, <a href="/search/physics?searchtype=author&amp;query=Bodenstein%2C+R+M">R. M. Bodenstein</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+S+A">S. A. Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Bruker%2C+M">M. Bruker</a>, <a href="/search/physics?searchtype=author&amp;query=Burrill%2C+A">A. Burrill</a>, <a href="/search/physics?searchtype=author&amp;query=Cardman%2C+L">L. Cardman</a>, <a href="/search/physics?searchtype=author&amp;query=Creel%2C+J">J. Creel</a>, <a href="/search/physics?searchtype=author&amp;query=Chao%2C+Y+-">Y. -C. Chao</a>, <a href="/search/physics?searchtype=author&amp;query=Cheng%2C+G">G. Cheng</a>, <a href="/search/physics?searchtype=author&amp;query=Ciovati%2C+G">G. Ciovati</a>, <a href="/search/physics?searchtype=author&amp;query=Chattopadhyay%2C+S">S. Chattopadhyay</a>, <a href="/search/physics?searchtype=author&amp;query=Clark%2C+J">J. Clark</a>, <a href="/search/physics?searchtype=author&amp;query=Clemens%2C+W+A">W. A. Clemens</a>, <a href="/search/physics?searchtype=author&amp;query=Croke%2C+G">G. Croke</a>, <a href="/search/physics?searchtype=author&amp;query=Daly%2C+E">E. Daly</a>, <a href="/search/physics?searchtype=author&amp;query=Davis%2C+G+K">G. K. Davis</a>, <a href="/search/physics?searchtype=author&amp;query=Delayen%2C+J">J. Delayen</a> , et al. (114 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="2408.16880v1-abstract-short" style="display: inline;"> This review paper describes the energy-upgraded CEBAF accelerator. This superconducting linac has achieved 12 GeV beam energy by adding 11 new high-performance cryomodules containing eighty-eight superconducting cavities that have operated CW at an average accelerating gradient of 20 MV/m. After reviewing the attributes and performance of the previous 6 GeV CEBAF accelerator, we discuss the upgrad&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2408.16880v1-abstract-full').style.display = 'inline'; document.getElementById('2408.16880v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2408.16880v1-abstract-full" style="display: none;"> This review paper describes the energy-upgraded CEBAF accelerator. This superconducting linac has achieved 12 GeV beam energy by adding 11 new high-performance cryomodules containing eighty-eight superconducting cavities that have operated CW at an average accelerating gradient of 20 MV/m. After reviewing the attributes and performance of the previous 6 GeV CEBAF accelerator, we discuss the upgraded CEBAF accelerator system in detail with particular attention paid to the new beam acceleration systems. In addition to doubling the acceleration in each linac, the upgrade included improving the beam recirculation magnets, adding more helium cooling capacity to allow the newly installed modules to run cold, adding a new experimental hall, and improving numerous other accelerator components. We review several of the techniques deployed to operate and analyze the accelerator performance, and document system operating experience and performance. In the final portion of the document, we present much of the current planning regarding projects to improve accelerator performance and enhance operating margins, and our plans for ensuring CEBAF operates reliably into the future. For the benefit of potential users of CEBAF, the performance and quality measures for beam delivered to each of the experimental halls is summarized in the appendix. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2408.16880v1-abstract-full').style.display = 'none'; document.getElementById('2408.16880v1-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 August, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2024. </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">66 pages, 73 figures, 21 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> JLAB-ACC-23-3940 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Accel. Beams 27 (2024) 084802 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2207.02095">arXiv:2207.02095</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2207.02095">pdf</a>, <a href="https://arxiv.org/format/2207.02095">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> The Development of Energy-Recovery Linacs </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adolphsen%2C+C">Chris Adolphsen</a>, <a href="/search/physics?searchtype=author&amp;query=Andre%2C+K">Kevin Andre</a>, <a href="/search/physics?searchtype=author&amp;query=Angal-Kalinin%2C+D">Deepa Angal-Kalinin</a>, <a href="/search/physics?searchtype=author&amp;query=Arnold%2C+M">Michaela Arnold</a>, <a href="/search/physics?searchtype=author&amp;query=Aulenbacher%2C+K">Kurt Aulenbacher</a>, <a href="/search/physics?searchtype=author&amp;query=Benson%2C+S">Steve Benson</a>, <a href="/search/physics?searchtype=author&amp;query=Bernauer%2C+J">Jan Bernauer</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+A">Alex Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Boonekamp%2C+M">Maarten Boonekamp</a>, <a href="/search/physics?searchtype=author&amp;query=Brinkmann%2C+R">Reinhard Brinkmann</a>, <a href="/search/physics?searchtype=author&amp;query=Bruker%2C+M">Max Bruker</a>, <a href="/search/physics?searchtype=author&amp;query=Br%C3%BCning%2C+O">Oliver Br眉ning</a>, <a href="/search/physics?searchtype=author&amp;query=Curatolo%2C+C">Camilla Curatolo</a>, <a href="/search/physics?searchtype=author&amp;query=Duthill%2C+P">Patxi Duthill</a>, <a href="/search/physics?searchtype=author&amp;query=Fischer%2C+O">Oliver Fischer</a>, <a href="/search/physics?searchtype=author&amp;query=Hoffstaetter%2C+G">Georg Hoffstaetter</a>, <a href="/search/physics?searchtype=author&amp;query=Holzer%2C+B">Bernhard Holzer</a>, <a href="/search/physics?searchtype=author&amp;query=Hounsell%2C+B">Ben Hounsell</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">Andrew Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Jensen%2C+E">Erk Jensen</a>, <a href="/search/physics?searchtype=author&amp;query=Kaabi%2C+W">Walid Kaabi</a>, <a href="/search/physics?searchtype=author&amp;query=Kayran%2C+D">Dmitry Kayran</a>, <a href="/search/physics?searchtype=author&amp;query=Klein%2C+M">Max Klein</a>, <a href="/search/physics?searchtype=author&amp;query=Knobloch%2C+J">Jens Knobloch</a>, <a href="/search/physics?searchtype=author&amp;query=Krafft%2C+G">Geoff Krafft</a> , et al. (24 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="2207.02095v2-abstract-short" style="display: inline;"> Energy-recovery linacs (ERLs) have been emphasised by the recent (2020) update of the European Strategy for Particle Physics as one of the most promising technologies for the accelerator base of future high-energy physics. The current paper has been written as a base document to support and specify details of the recently published European roadmap for the development of energy-recovery linacs. Th&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.02095v2-abstract-full').style.display = 'inline'; document.getElementById('2207.02095v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2207.02095v2-abstract-full" style="display: none;"> Energy-recovery linacs (ERLs) have been emphasised by the recent (2020) update of the European Strategy for Particle Physics as one of the most promising technologies for the accelerator base of future high-energy physics. The current paper has been written as a base document to support and specify details of the recently published European roadmap for the development of energy-recovery linacs. The paper summarises the previous achievements on ERLs and the status of the field and its basic technology items. The main possible future contributions and applications of ERLs to particle and nuclear physics as well as industrial developments are presented. The paper includes a vision for the further future, beyond 2030, as well as a comparative data base for the main existing and forthcoming ERL facilities. A series of continuous innovations, such as on intense electron sources or high-quality superconducting cavity technology, will massively contribute to the development of accelerator physics at large. Industrial applications are potentially revolutionary and may carry the development of ERLs much further, establishing another shining example of the impact of particle physics on society and its technical foundation with a special view on sustaining nature. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.02095v2-abstract-full').style.display = 'none'; document.getElementById('2207.02095v2-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 September, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 5 July, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2203.06164">arXiv:2203.06164</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2203.06164">pdf</a>, <a href="https://arxiv.org/ps/2203.06164">ps</a>, <a href="https://arxiv.org/format/2203.06164">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link 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="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> Higgs Factory Considerations </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Bagger%2C+J+A">J. A. Bagger</a>, <a href="/search/physics?searchtype=author&amp;query=Barish%2C+B+C">B. C. Barish</a>, <a href="/search/physics?searchtype=author&amp;query=Belomestnykh%2C+S">S. Belomestnykh</a>, <a href="/search/physics?searchtype=author&amp;query=Bhat%2C+P+C">P. C. Bhat</a>, <a href="/search/physics?searchtype=author&amp;query=Brau%2C+J+E">J. E. Brau</a>, <a href="/search/physics?searchtype=author&amp;query=Demarteau%2C+M">M. Demarteau</a>, <a href="/search/physics?searchtype=author&amp;query=Denisov%2C+D">D. Denisov</a>, <a href="/search/physics?searchtype=author&amp;query=Eno%2C+S+C">S. C. Eno</a>, <a href="/search/physics?searchtype=author&amp;query=Geddes%2C+C+G+R">C. G. R. Geddes</a>, <a href="/search/physics?searchtype=author&amp;query=Grannis%2C+P+D">P. D. Grannis</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Lankford%2C+A+J">A. J. Lankford</a>, <a href="/search/physics?searchtype=author&amp;query=Liepe%2C+M+U">M. U. Liepe</a>, <a href="/search/physics?searchtype=author&amp;query=MacFarlane%2C+D+B">D. B. MacFarlane</a>, <a href="/search/physics?searchtype=author&amp;query=Markiewicz%2C+T">T. Markiewicz</a>, <a href="/search/physics?searchtype=author&amp;query=Montgomery%2C+H+E">H. E. Montgomery</a>, <a href="/search/physics?searchtype=author&amp;query=Patterson%2C+J+R">J. R. Patterson</a>, <a href="/search/physics?searchtype=author&amp;query=Perelstein%2C+M">M. Perelstein</a>, <a href="/search/physics?searchtype=author&amp;query=Peskin%2C+M+E">M. E. Peskin</a>, <a href="/search/physics?searchtype=author&amp;query=Ross%2C+M+C">M. C. Ross</a>, <a href="/search/physics?searchtype=author&amp;query=Strube%2C+J">J. Strube</a>, <a href="/search/physics?searchtype=author&amp;query=White%2C+A+P">A. P. White</a>, <a href="/search/physics?searchtype=author&amp;query=Wilson%2C+G+W">G. W. Wilson</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="2203.06164v2-abstract-short" style="display: inline;"> We discuss considerations that can be used to formulate recommendations for initiating a lepton collider project that would provide precision studies of the Higgs boson and related electroweak phenomena. </span> <span class="abstract-full has-text-grey-dark mathjax" id="2203.06164v2-abstract-full" style="display: none;"> We discuss considerations that can be used to formulate recommendations for initiating a lepton collider project that would provide precision studies of the Higgs boson and related electroweak phenomena. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.06164v2-abstract-full').style.display = 'none'; document.getElementById('2203.06164v2-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 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">contribution to Snowmass 2021</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2201.07895">arXiv:2201.07895</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2201.07895">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link 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="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/10.23731/CYRM-2022-001">10.23731/CYRM-2022-001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> European Strategy for Particle Physics -- Accelerator R&amp;D Roadmap </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adolphsen%2C+C">C. Adolphsen</a>, <a href="/search/physics?searchtype=author&amp;query=Angal-Kalinin%2C+D">D. Angal-Kalinin</a>, <a href="/search/physics?searchtype=author&amp;query=Arndt%2C+T">T. Arndt</a>, <a href="/search/physics?searchtype=author&amp;query=Arnold%2C+M">M. Arnold</a>, <a href="/search/physics?searchtype=author&amp;query=Assmann%2C+R">R. Assmann</a>, <a href="/search/physics?searchtype=author&amp;query=Auchmann%2C+B">B. Auchmann</a>, <a href="/search/physics?searchtype=author&amp;query=Aulenbacher%2C+K">K. Aulenbacher</a>, <a href="/search/physics?searchtype=author&amp;query=Ballarino%2C+A">A. Ballarino</a>, <a href="/search/physics?searchtype=author&amp;query=Baudouy%2C+B">B. Baudouy</a>, <a href="/search/physics?searchtype=author&amp;query=Baudrenghien%2C+P">P. Baudrenghien</a>, <a href="/search/physics?searchtype=author&amp;query=Benedikt%2C+M">M. Benedikt</a>, <a href="/search/physics?searchtype=author&amp;query=Bentvelsen%2C+S">S. Bentvelsen</a>, <a href="/search/physics?searchtype=author&amp;query=Blondel%2C+A">A. Blondel</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+A">A. Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Bossi%2C+F">F. Bossi</a>, <a href="/search/physics?searchtype=author&amp;query=Bottura%2C+L">L. Bottura</a>, <a href="/search/physics?searchtype=author&amp;query=Bousson%2C+S">S. Bousson</a>, <a href="/search/physics?searchtype=author&amp;query=Br%C3%BCning%2C+O">O. Br眉ning</a>, <a href="/search/physics?searchtype=author&amp;query=Brinkmann%2C+R">R. Brinkmann</a>, <a href="/search/physics?searchtype=author&amp;query=Bruker%2C+M">M. Bruker</a>, <a href="/search/physics?searchtype=author&amp;query=Brunner%2C+O">O. Brunner</a>, <a href="/search/physics?searchtype=author&amp;query=Burrows%2C+P+N">P. N. Burrows</a>, <a href="/search/physics?searchtype=author&amp;query=Burt%2C+G">G. Burt</a>, <a href="/search/physics?searchtype=author&amp;query=Calatroni%2C+S">S. Calatroni</a>, <a href="/search/physics?searchtype=author&amp;query=Cassou%2C+K">K. Cassou</a> , et al. (111 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2201.07895v3-abstract-short" style="display: inline;"> The 2020 update of the European Strategy for Particle Physics emphasised the importance of an intensified and well-coordinated programme of accelerator R&amp;D, supporting the design and delivery of future particle accelerators in a timely, affordable and sustainable way. This report sets out a roadmap for European accelerator R&amp;D for the next five to ten years, covering five topical areas identified&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2201.07895v3-abstract-full').style.display = 'inline'; document.getElementById('2201.07895v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2201.07895v3-abstract-full" style="display: none;"> The 2020 update of the European Strategy for Particle Physics emphasised the importance of an intensified and well-coordinated programme of accelerator R&amp;D, supporting the design and delivery of future particle accelerators in a timely, affordable and sustainable way. This report sets out a roadmap for European accelerator R&amp;D for the next five to ten years, covering five topical areas identified in the Strategy update. The R&amp;D objectives include: improvement of the performance and cost-performance of magnet and radio-frequency acceleration systems; investigations of the potential of laser / plasma acceleration and energy-recovery linac techniques; and development of new concepts for muon beams and muon colliders. The goal of the roadmap is to document the collective view of the field on the next steps for the R&amp;D programme, and to provide the evidence base to support subsequent decisions on prioritisation, resourcing and implementation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2201.07895v3-abstract-full').style.display = 'none'; document.getElementById('2201.07895v3-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 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 19 January, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">270 pages, 58 figures. Editor: N. Mounet. LDG chair: D. Newbold. Panel chairs: P. V茅drine (HFM), S. Bousson (RF), R. Assmann (plasma), D. Schulte (muon), M. Klein (ERL). Panel editors: B. Baudouy (HFM), L. Bottura (HFM), S. Bousson (RF), G. Burt (RF), R. Assmann (plasma), E. Gschwendtner (plasma), R. Ischebeck (plasma), C. Rogers (muon), D. Schulte (muon), M. Klein (ERL)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CERN-2022-001 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> European Strategy for Particle Physics - Accelerator R&amp;D Roadmap, N. Mounet (ed.), CERN Yellow Reports: Monographs, CERN-2022-001 (CERN, Geneva, 2022) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2105.13564">arXiv:2105.13564</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2105.13564">pdf</a>, <a href="https://arxiv.org/format/2105.13564">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> Design concept for the second interaction region for Electron-Ion Collider </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Gamage%2C+B+R">B. R. Gamage</a>, <a href="/search/physics?searchtype=author&amp;query=Aschenauer%2C+E+-">E. -C. Aschenauer</a>, <a href="/search/physics?searchtype=author&amp;query=Berg%2C+J+S">J. S. Berg</a>, <a href="/search/physics?searchtype=author&amp;query=Burkert%2C+V">V. Burkert</a>, <a href="/search/physics?searchtype=author&amp;query=Ent%2C+R">R. Ent</a>, <a href="/search/physics?searchtype=author&amp;query=Furletova%2C+Y">Y. Furletova</a>, <a href="/search/physics?searchtype=author&amp;query=Higinbotham%2C+D">D. Higinbotham</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Hyde%2C+C">C. Hyde</a>, <a href="/search/physics?searchtype=author&amp;query=Jentsch%2C+A">A. Jentsch</a>, <a href="/search/physics?searchtype=author&amp;query=Kiselev%2C+A">A. Kiselev</a>, <a href="/search/physics?searchtype=author&amp;query=Lin%2C+F">F. Lin</a>, <a href="/search/physics?searchtype=author&amp;query=Michalski%2C+T">T. Michalski</a>, <a href="/search/physics?searchtype=author&amp;query=Montag%2C+C">C. Montag</a>, <a href="/search/physics?searchtype=author&amp;query=Morozov%2C+V+S">V. S. Morozov</a>, <a href="/search/physics?searchtype=author&amp;query=Nadel-Turonski%2C+P">P. Nadel-Turonski</a>, <a href="/search/physics?searchtype=author&amp;query=Palmer%2C+R">R. Palmer</a>, <a href="/search/physics?searchtype=author&amp;query=Parker%2C+B">B. Parker</a>, <a href="/search/physics?searchtype=author&amp;query=Ptitsyn%2C+V">V. Ptitsyn</a>, <a href="/search/physics?searchtype=author&amp;query=Rajput-Ghoshal%2C+R">R. Rajput-Ghoshal</a>, <a href="/search/physics?searchtype=author&amp;query=Romanov%2C+D">D. Romanov</a>, <a href="/search/physics?searchtype=author&amp;query=Satogata%2C+T">T. Satogata</a>, <a href="/search/physics?searchtype=author&amp;query=Seryi%2C+A">A. Seryi</a>, <a href="/search/physics?searchtype=author&amp;query=Sy%2C+A">A. Sy</a>, <a href="/search/physics?searchtype=author&amp;query=Weiss%2C+C">C. Weiss</a> , et al. (5 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="2105.13564v2-abstract-short" style="display: inline;"> The possibility of two interaction regions (IRs) is a design requirement for the Electron Ion Collider (the EIC). There is also a significant interest from the nuclear physics community in a 2nd IR with measurements capabilities complementary to those of the first IR. While the 2nd IR will be in operation over the entire energy range of ~20GeV to ~140GeV center of mass (CM). The 2nd IR can also pr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.13564v2-abstract-full').style.display = 'inline'; document.getElementById('2105.13564v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2105.13564v2-abstract-full" style="display: none;"> The possibility of two interaction regions (IRs) is a design requirement for the Electron Ion Collider (the EIC). There is also a significant interest from the nuclear physics community in a 2nd IR with measurements capabilities complementary to those of the first IR. While the 2nd IR will be in operation over the entire energy range of ~20GeV to ~140GeV center of mass (CM). The 2nd IR can also provide an acceptance coverage complementary to that of the first. We present a brief overview and the current progress of the 2nd IR design in terms of the parameters, magnet layout, and beam dynamics. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.13564v2-abstract-full').style.display = 'none'; document.getElementById('2105.13564v2-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 August, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 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">To be published in the proceedings of IPAC&#39;21</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2010.15791">arXiv:2010.15791</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2010.15791">pdf</a>, <a href="https://arxiv.org/format/2010.15791">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-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/PhysRevAccelBeams.24.012801">10.1103/PhysRevAccelBeams.24.012801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Demonstration of electron cooling using a pulsed beam from an electrostatic electron cooler </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Bruker%2C+M+W">M. W. Bruker</a>, <a href="/search/physics?searchtype=author&amp;query=Benson%2C+S">S. Benson</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Jordan%2C+K">K. Jordan</a>, <a href="/search/physics?searchtype=author&amp;query=Powers%2C+T">T. Powers</a>, <a href="/search/physics?searchtype=author&amp;query=Rimmer%2C+R">R. Rimmer</a>, <a href="/search/physics?searchtype=author&amp;query=Satogata%2C+T">T. Satogata</a>, <a href="/search/physics?searchtype=author&amp;query=Sy%2C+A">A. Sy</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+H">H. Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+S">S. Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Zhang%2C+H">H. Zhang</a>, <a href="/search/physics?searchtype=author&amp;query=Zhang%2C+Y">Y. Zhang</a>, <a href="/search/physics?searchtype=author&amp;query=Ma%2C+F">F. Ma</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+J">J. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Ma%2C+X+M">X. M. Ma</a>, <a href="/search/physics?searchtype=author&amp;query=Mao%2C+L+J">L. J. Mao</a>, <a href="/search/physics?searchtype=author&amp;query=Sha%2C+X+P">X. P. Sha</a>, <a href="/search/physics?searchtype=author&amp;query=Tang%2C+M+T">M. T. Tang</a>, <a href="/search/physics?searchtype=author&amp;query=Yang%2C+J+C">J. C. Yang</a>, <a href="/search/physics?searchtype=author&amp;query=Yang%2C+X+D">X. D. Yang</a>, <a href="/search/physics?searchtype=author&amp;query=Zhao%2C+H">H. Zhao</a>, <a href="/search/physics?searchtype=author&amp;query=Zhao%2C+H+W">H. W. Zhao</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="2010.15791v1-abstract-short" style="display: inline;"> Cooling of hadron beams is critically important in the next generation of hadron storage rings for delivery of unprecedented performance. One such application is the electron-ion collider presently under development in the US. The desire to develop electron coolers for operation at much higher energies than previously achieved necessitates the use of radio-frequency (RF) fields for acceleration as&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.15791v1-abstract-full').style.display = 'inline'; document.getElementById('2010.15791v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2010.15791v1-abstract-full" style="display: none;"> Cooling of hadron beams is critically important in the next generation of hadron storage rings for delivery of unprecedented performance. One such application is the electron-ion collider presently under development in the US. The desire to develop electron coolers for operation at much higher energies than previously achieved necessitates the use of radio-frequency (RF) fields for acceleration as opposed to the conventional, electrostatic approach. While electron cooling is a mature technology at low energy utilizing a DC beam, RF acceleration requires the cooling beam to be bunched, thus extending the parameter space to an unexplored territory. It is important to experimentally demonstrate the feasibility of cooling with electron bunches and further investigate how the relative time structure of the two beams affects the cooling properties; thus, a set of four pulsed-beam cooling experiments was carried out by a collaboration of Jefferson Lab and Institute of Modern Physics (IMP). The experiments have successfully demonstrated cooling with a beam of electron bunches in both the longitudinal and transverse directions for the first time. We have measured the effect of the electron bunch length and longitudinal ion focusing strength on the temporal evolution of the longitudinal and transverse ion beam profile and demonstrate that if the synchronization can be accurately maintained, the dynamics are not adversely affected by the change in time structure. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.15791v1-abstract-full').style.display = 'none'; document.getElementById('2010.15791v1-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 October, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">13 pages, 19 figures. Submitted to Physical Review Accelerators and Beams</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1903.01629">arXiv:1903.01629</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1903.01629">pdf</a>, <a href="https://arxiv.org/format/1903.01629">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link 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="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> The International Linear Collider: A Global Project </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Bambade%2C+P">Philip Bambade</a>, <a href="/search/physics?searchtype=author&amp;query=Barklow%2C+T">Tim Barklow</a>, <a href="/search/physics?searchtype=author&amp;query=Behnke%2C+T">Ties Behnke</a>, <a href="/search/physics?searchtype=author&amp;query=Berggren%2C+M">Mikael Berggren</a>, <a href="/search/physics?searchtype=author&amp;query=Brau%2C+J">James Brau</a>, <a href="/search/physics?searchtype=author&amp;query=Burrows%2C+P">Philip Burrows</a>, <a href="/search/physics?searchtype=author&amp;query=Denisov%2C+D">Dmitri Denisov</a>, <a href="/search/physics?searchtype=author&amp;query=Faus-Golfe%2C+A">Angeles Faus-Golfe</a>, <a href="/search/physics?searchtype=author&amp;query=Foster%2C+B">Brian Foster</a>, <a href="/search/physics?searchtype=author&amp;query=Fujii%2C+K">Keisuke Fujii</a>, <a href="/search/physics?searchtype=author&amp;query=Fuster%2C+J">Juan Fuster</a>, <a href="/search/physics?searchtype=author&amp;query=Gaede%2C+F">Frank Gaede</a>, <a href="/search/physics?searchtype=author&amp;query=Grannis%2C+P">Paul Grannis</a>, <a href="/search/physics?searchtype=author&amp;query=Grojean%2C+C">Christophe Grojean</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">Andrew Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=List%2C+B">Benno List</a>, <a href="/search/physics?searchtype=author&amp;query=List%2C+J">Jenny List</a>, <a href="/search/physics?searchtype=author&amp;query=Michizono%2C+S">Shinichiro Michizono</a>, <a href="/search/physics?searchtype=author&amp;query=Miyamoto%2C+A">Akiya Miyamoto</a>, <a href="/search/physics?searchtype=author&amp;query=Napoly%2C+O">Olivier Napoly</a>, <a href="/search/physics?searchtype=author&amp;query=Peskin%2C+M">Michael Peskin</a>, <a href="/search/physics?searchtype=author&amp;query=Poeschl%2C+R">Roman Poeschl</a>, <a href="/search/physics?searchtype=author&amp;query=Simon%2C+F">Frank Simon</a>, <a href="/search/physics?searchtype=author&amp;query=Strube%2C+J">Jan Strube</a>, <a href="/search/physics?searchtype=author&amp;query=Tian%2C+J">Junping Tian</a> , et al. (7 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="1903.01629v3-abstract-short" style="display: inline;"> The International Linear Collider (ILC) is now under consideration as the next global project in particle physics. In this report, we review of all aspects of the ILC program: the physics motivation, the accelerator design, the run plan, the proposed detectors, the experimental measurements on the Higgs boson, the top quark, the couplings of the W and Z bosons, and searches for new particles. We r&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1903.01629v3-abstract-full').style.display = 'inline'; document.getElementById('1903.01629v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1903.01629v3-abstract-full" style="display: none;"> The International Linear Collider (ILC) is now under consideration as the next global project in particle physics. In this report, we review of all aspects of the ILC program: the physics motivation, the accelerator design, the run plan, the proposed detectors, the experimental measurements on the Higgs boson, the top quark, the couplings of the W and Z bosons, and searches for new particles. We review the important role that polarized beams play in the ILC program. The first stage of the ILC is planned to be a Higgs factory at 250 GeV in the centre of mass. Energy upgrades can naturally be implemented based on the concept of a linear collider. We discuss in detail the ILC program of Higgs boson measurements and the expected precision in the determination of Higgs couplings. We compare the ILC capabilities to those of the HL-LHC and to those of other proposed e+e- Higgs factories. We emphasize throughout that the readiness of the accelerator and the estimates of ILC performance are based on detailed simulations backed by extensive RandD and, for the accelerator technology, operational experience. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1903.01629v3-abstract-full').style.display = 'none'; document.getElementById('1903.01629v3-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 April, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 March, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2019. </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">104 pages, 88 figures; v2: minor typo corrections; v3: many minor changes, including small corrections to the Tables and Figures in Section 11</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> DESY 19-037, FERMILAB-FN-1067-PPD, IFIC/19-10, IRFU-19-10, JLAB-PHY-19-2854, KEK Preprint 2018-92, LAL/RT 19-001, PNNL-SA-142168, SLAC-PUB-17412 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1901.09829">arXiv:1901.09829</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1901.09829">pdf</a>, <a href="https://arxiv.org/format/1901.09829">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link 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="Accelerator Physics">physics.acc-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> The International Linear Collider. A Global Project </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Aihara%2C+H">Hiroaki Aihara</a>, <a href="/search/physics?searchtype=author&amp;query=Bagger%2C+J">Jonathan Bagger</a>, <a href="/search/physics?searchtype=author&amp;query=Bambade%2C+P">Philip Bambade</a>, <a href="/search/physics?searchtype=author&amp;query=Barish%2C+B">Barry Barish</a>, <a href="/search/physics?searchtype=author&amp;query=Behnke%2C+T">Ties Behnke</a>, <a href="/search/physics?searchtype=author&amp;query=Bellerive%2C+A">Alain Bellerive</a>, <a href="/search/physics?searchtype=author&amp;query=Berggren%2C+M">Mikael Berggren</a>, <a href="/search/physics?searchtype=author&amp;query=Brau%2C+J">James Brau</a>, <a href="/search/physics?searchtype=author&amp;query=Breidenbach%2C+M">Martin Breidenbach</a>, <a href="/search/physics?searchtype=author&amp;query=Bozovic-Jelisavcic%2C+I">Ivanka Bozovic-Jelisavcic</a>, <a href="/search/physics?searchtype=author&amp;query=Burrows%2C+P">Philip Burrows</a>, <a href="/search/physics?searchtype=author&amp;query=Caccia%2C+M">Massimo Caccia</a>, <a href="/search/physics?searchtype=author&amp;query=Colas%2C+P">Paul Colas</a>, <a href="/search/physics?searchtype=author&amp;query=Denisov%2C+D">Dmitri Denisov</a>, <a href="/search/physics?searchtype=author&amp;query=Eigen%2C+G">Gerald Eigen</a>, <a href="/search/physics?searchtype=author&amp;query=Evans%2C+L">Lyn Evans</a>, <a href="/search/physics?searchtype=author&amp;query=Faus-Golfe%2C+A">Angeles Faus-Golfe</a>, <a href="/search/physics?searchtype=author&amp;query=Foster%2C+B">Brian Foster</a>, <a href="/search/physics?searchtype=author&amp;query=Fujii%2C+K">Keisuke Fujii</a>, <a href="/search/physics?searchtype=author&amp;query=Fuster%2C+J">Juan Fuster</a>, <a href="/search/physics?searchtype=author&amp;query=Gaede%2C+F">Frank Gaede</a>, <a href="/search/physics?searchtype=author&amp;query=Gao%2C+J">Jie Gao</a>, <a href="/search/physics?searchtype=author&amp;query=Grannis%2C+P">Paul Grannis</a>, <a href="/search/physics?searchtype=author&amp;query=Grojean%2C+C">Christophe Grojean</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">Andrew Hutton</a> , et al. (37 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="1901.09829v1-abstract-short" style="display: inline;"> A large, world-wide community of physicists is working to realise an exceptional physics program of energy-frontier, electron-positron collisions with the International Linear Collider (ILC). This program will begin with a central focus on high-precision and model-independent measurements of the Higgs boson couplings. This method of searching for new physics beyond the Standard Model is orthogonal&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.09829v1-abstract-full').style.display = 'inline'; document.getElementById('1901.09829v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1901.09829v1-abstract-full" style="display: none;"> A large, world-wide community of physicists is working to realise an exceptional physics program of energy-frontier, electron-positron collisions with the International Linear Collider (ILC). This program will begin with a central focus on high-precision and model-independent measurements of the Higgs boson couplings. This method of searching for new physics beyond the Standard Model is orthogonal to and complements the LHC physics program. The ILC at 250 GeV will also search for direct new physics in exotic Higgs decays and in pair-production of weakly interacting particles. Polarised electron and positron beams add unique opportunities to the physics reach. The ILC can be upgraded to higher energy, enabling precision studies of the top quark and measurement of the top Yukawa coupling and the Higgs self-coupling. The key accelerator technology, superconducting radio-frequency cavities, has matured. Optimised collider and detector designs, and associated physics analyses, were presented in the ILC Technical Design Report, signed by 2400 scientists. There is a strong interest in Japan to host this international effort. A detailed review of the many aspects of the project is nearing a conclusion in Japan. Now the Japanese government is preparing for a decision on the next phase of international negotiations, that could lead to a project start within a few years. The potential timeline of the ILC project includes an initial phase of about 4 years to obtain international agreements, complete engineering design and prepare construction, and form the requisite international collaboration, followed by a construction phase of 9 years. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.09829v1-abstract-full').style.display = 'none'; document.getElementById('1901.09829v1-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 January, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2019. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1705.08783">arXiv:1705.08783</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1705.08783">pdf</a>, <a href="https://arxiv.org/format/1705.08783">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-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/10.1088/1361-6471/aaa171">10.1088/1361-6471/aaa171 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> PERLE: Powerful Energy Recovery Linac for Experiments - Conceptual Design Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Angal-Kalinin%2C+D">D. Angal-Kalinin</a>, <a href="/search/physics?searchtype=author&amp;query=Arduini%2C+G">G. Arduini</a>, <a href="/search/physics?searchtype=author&amp;query=Auchmann%2C+B">B. Auchmann</a>, <a href="/search/physics?searchtype=author&amp;query=Bernauer%2C+J">J. Bernauer</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+A">A. Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Bordry%2C+F">F. Bordry</a>, <a href="/search/physics?searchtype=author&amp;query=Bousson%2C+S">S. Bousson</a>, <a href="/search/physics?searchtype=author&amp;query=Bracco%2C+C">C. Bracco</a>, <a href="/search/physics?searchtype=author&amp;query=Br%C3%BCning%2C+O">O. Br眉ning</a>, <a href="/search/physics?searchtype=author&amp;query=Calaga%2C+R">R. Calaga</a>, <a href="/search/physics?searchtype=author&amp;query=Cassou%2C+K">K. Cassou</a>, <a href="/search/physics?searchtype=author&amp;query=Chetvertkova%2C+V">V. Chetvertkova</a>, <a href="/search/physics?searchtype=author&amp;query=Cormier%2C+E">E. Cormier</a>, <a href="/search/physics?searchtype=author&amp;query=Daly%2C+E">E. Daly</a>, <a href="/search/physics?searchtype=author&amp;query=Douglas%2C+D">D. Douglas</a>, <a href="/search/physics?searchtype=author&amp;query=Dupraz%2C+K">K. Dupraz</a>, <a href="/search/physics?searchtype=author&amp;query=Goddard%2C+B">B. Goddard</a>, <a href="/search/physics?searchtype=author&amp;query=Henry%2C+J">J. Henry</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Jensen%2C+E">E. Jensen</a>, <a href="/search/physics?searchtype=author&amp;query=Kaabi%2C+W">W. Kaabi</a>, <a href="/search/physics?searchtype=author&amp;query=Klein%2C+M">M. Klein</a>, <a href="/search/physics?searchtype=author&amp;query=Kostka%2C+P">P. Kostka</a>, <a href="/search/physics?searchtype=author&amp;query=Marhauser%2C+F">F. Marhauser</a>, <a href="/search/physics?searchtype=author&amp;query=Martens%2C+A">A. Martens</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="1705.08783v1-abstract-short" style="display: inline;"> A conceptual design is presented of a novel ERL facility for the development and application of the energy recovery technique to linear electron accelerators in the multi-turn, large current and large energy regime. The main characteristics of the powerful energy recovery linac experiment facility (PERLE) are derived from the design of the Large Hadron electron Collider, an electron beam upgrade u&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1705.08783v1-abstract-full').style.display = 'inline'; document.getElementById('1705.08783v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1705.08783v1-abstract-full" style="display: none;"> A conceptual design is presented of a novel ERL facility for the development and application of the energy recovery technique to linear electron accelerators in the multi-turn, large current and large energy regime. The main characteristics of the powerful energy recovery linac experiment facility (PERLE) are derived from the design of the Large Hadron electron Collider, an electron beam upgrade under study for the LHC, for which it would be the key demonstrator. PERLE is thus projected as a facility to investigate efficient, high current (&gt; 10 mA) ERL operation with three re-circulation passages through newly designed SCRF cavities, at 801.58 MHz frequency, and following deceleration over another three re-circulations. In its fully equipped configuration, PERLE provides an electron beam of approximately 1 GeV energy. A physics programme possibly associated with PERLE is sketched, consisting of high precision elastic electron-proton scattering experiments, as well as photo-nuclear reactions of unprecedented intensities with up to 30 MeV photon beam energy as may be obtained using Fabry-Perot cavities. The facility has further applications as a general technology test bed that can investigate and validate novel superconducting magnets (beam induced quench tests) and superconducting RF structures (structure tests with high current beams, beam loading and transients). Besides a chapter on operation aspects, the report contains detailed considerations on the choices for the SCRF structure, optics and lattice design, solutions for arc magnets, source and injector and on further essential components. A suitable configuration derived from the here presented design concept may next be moved forward to a technical design and possibly be built by an international collaboration which is being established. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1705.08783v1-abstract-full').style.display = 'none'; document.getElementById('1705.08783v1-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 May, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2017. </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">112 pages, 63 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/1606.09117">arXiv:1606.09117</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1606.09117">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> Study of Beam Synchronization at JLEIC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Morozov%2C+V+S">V. S. Morozov</a>, <a href="/search/physics?searchtype=author&amp;query=Derbenev%2C+Y+S">Ya. S. Derbenev</a>, <a href="/search/physics?searchtype=author&amp;query=Guo%2C+J">J. Guo</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Lin%2C+F">F. Lin</a>, <a href="/search/physics?searchtype=author&amp;query=Michalski%2C+T">T. Michalski</a>, <a href="/search/physics?searchtype=author&amp;query=Nadel-Turonski%2C+P">P. Nadel-Turonski</a>, <a href="/search/physics?searchtype=author&amp;query=Pilat%2C+F">F. Pilat</a>, <a href="/search/physics?searchtype=author&amp;query=Rimmer%2C+R">R. Rimmer</a>, <a href="/search/physics?searchtype=author&amp;query=Satogata%2C+T">T. Satogata</a>, <a href="/search/physics?searchtype=author&amp;query=Wang%2C+H">H. Wang</a>, <a href="/search/physics?searchtype=author&amp;query=Zhang%2C+Y">Y. Zhang</a>, <a href="/search/physics?searchtype=author&amp;query=Terzic%2C+B">B. Terzic</a>, <a href="/search/physics?searchtype=author&amp;query=Wienands%2C+U">U. Wienands</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="1606.09117v1-abstract-short" style="display: inline;"> The ion collider ring of Jefferson Lab Electron-Ion Collider (JLEIC) accommodates a wide range of ion energies, from 20 to 100 GeV for protons or from 8 to 40 GeV per nucleon for lead ions. In this medium energy range, ions are not fully relativistic, which means values of their relativistic beta are slightly below 1, leading to an energy dependence of revolution time of the collider ring. On the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.09117v1-abstract-full').style.display = 'inline'; document.getElementById('1606.09117v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1606.09117v1-abstract-full" style="display: none;"> The ion collider ring of Jefferson Lab Electron-Ion Collider (JLEIC) accommodates a wide range of ion energies, from 20 to 100 GeV for protons or from 8 to 40 GeV per nucleon for lead ions. In this medium energy range, ions are not fully relativistic, which means values of their relativistic beta are slightly below 1, leading to an energy dependence of revolution time of the collider ring. On the other hand, electrons with energy 3 GeV and above are already ultra-relativistic such that their speeds are effectively equal to the speed of light. The difference in speeds of colliding electrons and ions in JLEIC, when translated into a path-length difference necessary to maintain the same timing between electron and ion bunches, is quite large. In this paper, we explore schemes for synchronizing the electron and ion bunches at a collision point as the ion energy is varied. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1606.09117v1-abstract-full').style.display = 'none'; document.getElementById('1606.09117v1-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 June, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1504.07961">arXiv:1504.07961</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1504.07961">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> MEIC Design Summary </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Abeyratne%2C+S">S. Abeyratne</a>, <a href="/search/physics?searchtype=author&amp;query=Barber%2C+D">D. Barber</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+A">A. Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Brindza%2C+P">P. Brindza</a>, <a href="/search/physics?searchtype=author&amp;query=Cai%2C+Y">Y. Cai</a>, <a href="/search/physics?searchtype=author&amp;query=Camsonne%2C+A">A. Camsonne</a>, <a href="/search/physics?searchtype=author&amp;query=Castilla%2C+A">A. Castilla</a>, <a href="/search/physics?searchtype=author&amp;query=Chevtsov%2C+P">P. Chevtsov</a>, <a href="/search/physics?searchtype=author&amp;query=Daly%2C+E">E. Daly</a>, <a href="/search/physics?searchtype=author&amp;query=Derbenev%2C+Y+S">Y. S. Derbenev</a>, <a href="/search/physics?searchtype=author&amp;query=Douglas%2C+D">D. Douglas</a>, <a href="/search/physics?searchtype=author&amp;query=Dudnikov%2C+V">V. Dudnikov</a>, <a href="/search/physics?searchtype=author&amp;query=Ent%2C+R">R. Ent</a>, <a href="/search/physics?searchtype=author&amp;query=Erdelyi%2C+B">B. Erdelyi</a>, <a href="/search/physics?searchtype=author&amp;query=Filatov%2C+Y">Y. Filatov</a>, <a href="/search/physics?searchtype=author&amp;query=Gaskell%2C+D">D. Gaskell</a>, <a href="/search/physics?searchtype=author&amp;query=Grames%2C+J">J. Grames</a>, <a href="/search/physics?searchtype=author&amp;query=Guo%2C+J">J. Guo</a>, <a href="/search/physics?searchtype=author&amp;query=Harwood%2C+L">L. Harwood</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Hyde%2C+C">C. Hyde</a>, <a href="/search/physics?searchtype=author&amp;query=Jordan%2C+K">K. Jordan</a>, <a href="/search/physics?searchtype=author&amp;query=Kimber%2C+A">A. Kimber</a>, <a href="/search/physics?searchtype=author&amp;query=Krafft%2C+G+A">G. A. Krafft</a>, <a href="/search/physics?searchtype=author&amp;query=Kondratenko%2C+A">A. Kondratenko</a> , et al. (30 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="1504.07961v1-abstract-short" style="display: inline;"> This document summarizes the design of Jefferson Lab&#39;s electron-ion collider, MEIC, as of January 20, 2015, and describes the facility whose cost was estimated for the United States Department of Energy Nuclear Sciences Advisory Committee EIC cost review of January 26-28, 2015. In particular, each of the main technical systems within the collider is presented to the level of the best current infor&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.07961v1-abstract-full').style.display = 'inline'; document.getElementById('1504.07961v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1504.07961v1-abstract-full" style="display: none;"> This document summarizes the design of Jefferson Lab&#39;s electron-ion collider, MEIC, as of January 20, 2015, and describes the facility whose cost was estimated for the United States Department of Energy Nuclear Sciences Advisory Committee EIC cost review of January 26-28, 2015. In particular, each of the main technical systems within the collider is presented to the level of the best current information. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.07961v1-abstract-full').style.display = 'none'; document.getElementById('1504.07961v1-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, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2015. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1403.2318">arXiv:1403.2318</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1403.2318">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> Control of Coherent Synchrotron Radiation and Micro-Bunching Effects During Transport of High Brightness Electron Beams </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Douglas%2C+D+R">D. R. Douglas</a>, <a href="/search/physics?searchtype=author&amp;query=Benson%2C+S+V">S. V. Benson</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a>, <a href="/search/physics?searchtype=author&amp;query=Krafft%2C+G+A">G. A. Krafft</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+R">R. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Neil%2C+G+R">G. R. Neil</a>, <a href="/search/physics?searchtype=author&amp;query=Roblin%2C+Y">Y. Roblin</a>, <a href="/search/physics?searchtype=author&amp;query=Tennant%2C+C+D">C. D. Tennant</a>, <a href="/search/physics?searchtype=author&amp;query=Tsai%2C+C+-">C. -Y. Tsai</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="1403.2318v1-abstract-short" style="display: inline;"> Beam quality preservation during transport of high-brightness electron beams is of general concern in the design of modern accelerators. Methods to manage incoherent synchrotron radiation (ISR) have been in place for decades; as beam brightness has improved coherent synchrotron radiation (CSR) and the microbunching instability (uBI) have emerged as performance limitations. We apply the compensatio&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1403.2318v1-abstract-full').style.display = 'inline'; document.getElementById('1403.2318v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1403.2318v1-abstract-full" style="display: none;"> Beam quality preservation during transport of high-brightness electron beams is of general concern in the design of modern accelerators. Methods to manage incoherent synchrotron radiation (ISR) have been in place for decades; as beam brightness has improved coherent synchrotron radiation (CSR) and the microbunching instability (uBI) have emerged as performance limitations. We apply the compensation analysis of diMitri, Cornacchia, and Spampinati - as previously used by Borland - to the design of transport systems for use with low-emittance beams, and find that appropriately configured second order achromats will suppress transverse emittance growth due to CSR and appear to limit uBI gain. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1403.2318v1-abstract-full').style.display = 'none'; document.getElementById('1403.2318v1-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> 10 March, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2014. </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">27 pages, 31 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> JLAB-ACP-14-1751 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1209.0757">arXiv:1209.0757</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.0757">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link 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="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Science Requirements and Conceptual Design for a Polarized Medium Energy Electron-Ion Collider at Jefferson Lab </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Abeyratne%2C+S">S. Abeyratne</a>, <a href="/search/physics?searchtype=author&amp;query=Accardi%2C+A">A. Accardi</a>, <a href="/search/physics?searchtype=author&amp;query=Ahmed%2C+S">S. Ahmed</a>, <a href="/search/physics?searchtype=author&amp;query=Barber%2C+D">D. Barber</a>, <a href="/search/physics?searchtype=author&amp;query=Bisognano%2C+J">J. Bisognano</a>, <a href="/search/physics?searchtype=author&amp;query=Bogacz%2C+A">A. Bogacz</a>, <a href="/search/physics?searchtype=author&amp;query=Castilla%2C+A">A. Castilla</a>, <a href="/search/physics?searchtype=author&amp;query=Chevtsov%2C+P">P. Chevtsov</a>, <a href="/search/physics?searchtype=author&amp;query=Corneliussen%2C+S">S. Corneliussen</a>, <a href="/search/physics?searchtype=author&amp;query=Deconinck%2C+W">W. Deconinck</a>, <a href="/search/physics?searchtype=author&amp;query=Degtiarenko%2C+P">P. Degtiarenko</a>, <a href="/search/physics?searchtype=author&amp;query=Delayen%2C+J">J. Delayen</a>, <a href="/search/physics?searchtype=author&amp;query=Derbenev%2C+Y">Ya. Derbenev</a>, <a href="/search/physics?searchtype=author&amp;query=DeSilva%2C+S">S. DeSilva</a>, <a href="/search/physics?searchtype=author&amp;query=Douglas%2C+D">D. Douglas</a>, <a href="/search/physics?searchtype=author&amp;query=Dudnikov%2C+V">V. Dudnikov</a>, <a href="/search/physics?searchtype=author&amp;query=Ent%2C+R">R. Ent</a>, <a href="/search/physics?searchtype=author&amp;query=Erdelyi%2C+B">B. Erdelyi</a>, <a href="/search/physics?searchtype=author&amp;query=Evtushenko%2C+P">P. Evtushenko</a>, <a href="/search/physics?searchtype=author&amp;query=Filatov%2C+Y">Yu. Filatov</a>, <a href="/search/physics?searchtype=author&amp;query=Gaskell%2C+D">D. Gaskell</a>, <a href="/search/physics?searchtype=author&amp;query=Geng%2C+R">R. Geng</a>, <a href="/search/physics?searchtype=author&amp;query=Guzey%2C+V">V. Guzey</a>, <a href="/search/physics?searchtype=author&amp;query=Horn%2C+T">T. Horn</a>, <a href="/search/physics?searchtype=author&amp;query=Hutton%2C+A">A. Hutton</a> , et al. (33 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="1209.0757v2-abstract-short" style="display: inline;"> This report presents a brief summary of the science opportunities and program of a polarized medium energy electron-ion collider at Jefferson Lab and a comprehensive description of the conceptual design of such a collider based on the CEBAF electron accelerator facility. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.0757v2-abstract-full" style="display: none;"> This report presents a brief summary of the science opportunities and program of a polarized medium energy electron-ion collider at Jefferson Lab and a comprehensive description of the conceptual design of such a collider based on the CEBAF electron accelerator facility. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.0757v2-abstract-full').style.display = 'none'; document.getElementById('1209.0757v2-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, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">160 pages, ~93 figures This work was supported by the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC05-06OR23177, DE-AC02-06CH11357, DE-AC05-060R23177, and DESC0005823. The U.S. Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce this manuscript for U.S. Government purposes</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> JLAB-ACC-12-1619 </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" 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