New Horizons: Scalar and Vector Ultralight Dark Matter
The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. Transformative advances in quantum technologies have led to a plethora of new high-precision quantum sensors and dark matter detection strategi...
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creator | Banerjee, A Bartram, C Baryakhtar, M Betz, J Boutan, C Bowring, D Budker, D Carney, D Carosi, G Chaudhuri, S Chowdhury, M. D Co, R. T Demarteau, M DePorzio, N Derbin, A. V Deshpande, T Di Luzio, L Diaz-Morcillo, A Doyle, J. M Drlica-Wagner, A Droster, A Du, N Döbrich, B Eby, J Essig, R Figueroa, N. L Fry, J. T Gardner, S Geraci, A. A Ghosh, S Giannotti, M Gimeno, B Griffin, S. M Grin, D Grote, H Gundlach, J. H Guzzetti, M Hanneke, D Harnik, R Henning, R Irsic, V Jackson, H Kimball, D. F. Jackson Jaeckel, J Kagan, M Khatiwada, R Knirck, S Kovachy, T Kuenstner, S. E Lasner, Z Leder, A. F Lehnert, R Leibrandt, D. R Lewis, S. M Manley, J Maruyama, R. H Muratova, V. N O'Hare, C. A. J Ouellet, J. L Pappas, K. M. W Peik, E Perez, G Robles, V. H Safdari, M Safronova, M. S Salemi, C. P Schmidt, P. O Schumm, T Schwartzman, A Shu, J Simanovskaia, M Smith, M. S Snow, W. M Stadnik, Y. V Sun, C Sushkov, A. O Tait, T. M. P Takhistov, V Tanner, D. B Temples, D. J Thomas, J. H Tobar, M. E Tretiak, O Tsai, Y. -D Tyson, J. A Vandegar, M Vermeulen, S Visinelli, L Wang, Z Wilson, D. J Winslow, L Withington, S Yang, J Ye, J Young, B. A Yu, F Zaheer, M. H Zelevinsky, T Zhao, Y Zhou, K |
description | The last decade has seen unprecedented effort in dark matter model building
at all mass scales coupled with the design of numerous new detection
strategies. Transformative advances in quantum technologies have led to a
plethora of new high-precision quantum sensors and dark matter detection
strategies for ultralight ($ |
doi_str_mv | 10.48550/arxiv.2203.14915 |
format | Article |
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at all mass scales coupled with the design of numerous new detection
strategies. Transformative advances in quantum technologies have led to a
plethora of new high-precision quantum sensors and dark matter detection
strategies for ultralight ($<10\,$eV) bosonic dark matter that can be described
by an oscillating classical, largely coherent field. This white paper focuses
on searches for wavelike scalar and vector dark matter candidates.</description><identifier>DOI: 10.48550/arxiv.2203.14915</identifier><language>eng</language><subject>Physics - Cosmology and Nongalactic Astrophysics ; Physics - High Energy Physics - Experiment ; Physics - High Energy Physics - Phenomenology ; Physics - Instrumentation and Detectors ; Physics - Quantum Physics</subject><creationdate>2022-03</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2203.14915$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2203.14915$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Banerjee, A</creatorcontrib><creatorcontrib>Bartram, C</creatorcontrib><creatorcontrib>Baryakhtar, M</creatorcontrib><creatorcontrib>Betz, J</creatorcontrib><creatorcontrib>Boutan, C</creatorcontrib><creatorcontrib>Bowring, D</creatorcontrib><creatorcontrib>Budker, D</creatorcontrib><creatorcontrib>Carney, D</creatorcontrib><creatorcontrib>Carosi, G</creatorcontrib><creatorcontrib>Chaudhuri, S</creatorcontrib><creatorcontrib>Chowdhury, M. 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H</creatorcontrib><creatorcontrib>Zelevinsky, T</creatorcontrib><creatorcontrib>Zhao, Y</creatorcontrib><creatorcontrib>Zhou, K</creatorcontrib><title>New Horizons: Scalar and Vector Ultralight Dark Matter</title><description>The last decade has seen unprecedented effort in dark matter model building
at all mass scales coupled with the design of numerous new detection
strategies. Transformative advances in quantum technologies have led to a
plethora of new high-precision quantum sensors and dark matter detection
strategies for ultralight ($<10\,$eV) bosonic dark matter that can be described
by an oscillating classical, largely coherent field. This white paper focuses
on searches for wavelike scalar and vector dark matter candidates.</description><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Physics - Instrumentation and Detectors</subject><subject>Physics - Quantum Physics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj8tOwzAQAH3pARU-gBP-gQQn613H3FB5FKktBwrXaOPaNCI0aGvx-npE4TS30YxSp5UpbYNozlk--_eyrg2UlfUVHilaxQ89H6X_Hnf7C_0QeGDRvNvopxjyKPpxyMJD_7zN-orlRS855yjHapJ42MeTf07V-uZ6PZsXi_vbu9nlomByWLAn14A3HW6QugiYwDhviJINtgkxgQMf6xQ4Ilm0jjpX1QQQ0XY2OJiqsz_tIbx9k_6V5av9HWgPA_ADYBo-wA</recordid><startdate>20220328</startdate><enddate>20220328</enddate><creator>Banerjee, A</creator><creator>Bartram, C</creator><creator>Baryakhtar, M</creator><creator>Betz, J</creator><creator>Boutan, C</creator><creator>Bowring, D</creator><creator>Budker, D</creator><creator>Carney, D</creator><creator>Carosi, G</creator><creator>Chaudhuri, S</creator><creator>Chowdhury, M. 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H</creator><creator>Zelevinsky, T</creator><creator>Zhao, Y</creator><creator>Zhou, K</creator><scope>GOX</scope></search><sort><creationdate>20220328</creationdate><title>New Horizons: Scalar and Vector Ultralight Dark Matter</title><author>Banerjee, A ; Bartram, C ; Baryakhtar, M ; Betz, J ; Boutan, C ; Bowring, D ; Budker, D ; Carney, D ; Carosi, G ; Chaudhuri, S ; Chowdhury, M. D ; Co, R. T ; Demarteau, M ; DePorzio, N ; Derbin, A. V ; Deshpande, T ; Di Luzio, L ; Diaz-Morcillo, A ; Doyle, J. M ; Drlica-Wagner, A ; Droster, A ; Du, N ; Döbrich, B ; Eby, J ; Essig, R ; Figueroa, N. L ; Fry, J. T ; Gardner, S ; Geraci, A. A ; Ghosh, S ; Giannotti, M ; Gimeno, B ; Griffin, S. M ; Grin, D ; Grote, H ; Gundlach, J. H ; Guzzetti, M ; Hanneke, D ; Harnik, R ; Henning, R ; Irsic, V ; Jackson, H ; Kimball, D. F. Jackson ; Jaeckel, J ; Kagan, M ; Khatiwada, R ; Knirck, S ; Kovachy, T ; Kuenstner, S. E ; Lasner, Z ; Leder, A. F ; Lehnert, R ; Leibrandt, D. R ; Lewis, S. M ; Manley, J ; Maruyama, R. H ; Muratova, V. N ; O'Hare, C. A. J ; Ouellet, J. L ; Pappas, K. M. W ; Peik, E ; Perez, G ; Robles, V. H ; Safdari, M ; Safronova, M. S ; Salemi, C. P ; Schmidt, P. O ; Schumm, T ; Schwartzman, A ; Shu, J ; Simanovskaia, M ; Smith, M. S ; Snow, W. M ; Stadnik, Y. V ; Sun, C ; Sushkov, A. O ; Tait, T. M. P ; Takhistov, V ; Tanner, D. B ; Temples, D. J ; Thomas, J. H ; Tobar, M. E ; Tretiak, O ; Tsai, Y. -D ; Tyson, J. A ; Vandegar, M ; Vermeulen, S ; Visinelli, L ; Wang, Z ; Wilson, D. J ; Winslow, L ; Withington, S ; Yang, J ; Ye, J ; Young, B. A ; Yu, F ; Zaheer, M. 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O</creatorcontrib><creatorcontrib>Tait, T. M. P</creatorcontrib><creatorcontrib>Takhistov, V</creatorcontrib><creatorcontrib>Tanner, D. B</creatorcontrib><creatorcontrib>Temples, D. J</creatorcontrib><creatorcontrib>Thomas, J. H</creatorcontrib><creatorcontrib>Tobar, M. E</creatorcontrib><creatorcontrib>Tretiak, O</creatorcontrib><creatorcontrib>Tsai, Y. -D</creatorcontrib><creatorcontrib>Tyson, J. A</creatorcontrib><creatorcontrib>Vandegar, M</creatorcontrib><creatorcontrib>Vermeulen, S</creatorcontrib><creatorcontrib>Visinelli, L</creatorcontrib><creatorcontrib>Wang, Z</creatorcontrib><creatorcontrib>Wilson, D. J</creatorcontrib><creatorcontrib>Winslow, L</creatorcontrib><creatorcontrib>Withington, S</creatorcontrib><creatorcontrib>Yang, J</creatorcontrib><creatorcontrib>Ye, J</creatorcontrib><creatorcontrib>Young, B. A</creatorcontrib><creatorcontrib>Yu, F</creatorcontrib><creatorcontrib>Zaheer, M. H</creatorcontrib><creatorcontrib>Zelevinsky, T</creatorcontrib><creatorcontrib>Zhao, Y</creatorcontrib><creatorcontrib>Zhou, K</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Banerjee, A</au><au>Bartram, C</au><au>Baryakhtar, M</au><au>Betz, J</au><au>Boutan, C</au><au>Bowring, D</au><au>Budker, D</au><au>Carney, D</au><au>Carosi, G</au><au>Chaudhuri, S</au><au>Chowdhury, M. D</au><au>Co, R. T</au><au>Demarteau, M</au><au>DePorzio, N</au><au>Derbin, A. V</au><au>Deshpande, T</au><au>Di Luzio, L</au><au>Diaz-Morcillo, A</au><au>Doyle, J. M</au><au>Drlica-Wagner, A</au><au>Droster, A</au><au>Du, N</au><au>Döbrich, B</au><au>Eby, J</au><au>Essig, R</au><au>Figueroa, N. L</au><au>Fry, J. T</au><au>Gardner, S</au><au>Geraci, A. A</au><au>Ghosh, S</au><au>Giannotti, M</au><au>Gimeno, B</au><au>Griffin, S. M</au><au>Grin, D</au><au>Grote, H</au><au>Gundlach, J. H</au><au>Guzzetti, M</au><au>Hanneke, D</au><au>Harnik, R</au><au>Henning, R</au><au>Irsic, V</au><au>Jackson, H</au><au>Kimball, D. F. Jackson</au><au>Jaeckel, J</au><au>Kagan, M</au><au>Khatiwada, R</au><au>Knirck, S</au><au>Kovachy, T</au><au>Kuenstner, S. E</au><au>Lasner, Z</au><au>Leder, A. F</au><au>Lehnert, R</au><au>Leibrandt, D. R</au><au>Lewis, S. M</au><au>Manley, J</au><au>Maruyama, R. H</au><au>Muratova, V. N</au><au>O'Hare, C. A. J</au><au>Ouellet, J. L</au><au>Pappas, K. M. W</au><au>Peik, E</au><au>Perez, G</au><au>Robles, V. H</au><au>Safdari, M</au><au>Safronova, M. S</au><au>Salemi, C. P</au><au>Schmidt, P. O</au><au>Schumm, T</au><au>Schwartzman, A</au><au>Shu, J</au><au>Simanovskaia, M</au><au>Smith, M. S</au><au>Snow, W. M</au><au>Stadnik, Y. V</au><au>Sun, C</au><au>Sushkov, A. O</au><au>Tait, T. M. P</au><au>Takhistov, V</au><au>Tanner, D. B</au><au>Temples, D. J</au><au>Thomas, J. H</au><au>Tobar, M. E</au><au>Tretiak, O</au><au>Tsai, Y. -D</au><au>Tyson, J. A</au><au>Vandegar, M</au><au>Vermeulen, S</au><au>Visinelli, L</au><au>Wang, Z</au><au>Wilson, D. J</au><au>Winslow, L</au><au>Withington, S</au><au>Yang, J</au><au>Ye, J</au><au>Young, B. A</au><au>Yu, F</au><au>Zaheer, M. H</au><au>Zelevinsky, T</au><au>Zhao, Y</au><au>Zhou, K</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New Horizons: Scalar and Vector Ultralight Dark Matter</atitle><date>2022-03-28</date><risdate>2022</risdate><abstract>The last decade has seen unprecedented effort in dark matter model building
at all mass scales coupled with the design of numerous new detection
strategies. Transformative advances in quantum technologies have led to a
plethora of new high-precision quantum sensors and dark matter detection
strategies for ultralight ($<10\,$eV) bosonic dark matter that can be described
by an oscillating classical, largely coherent field. This white paper focuses
on searches for wavelike scalar and vector dark matter candidates.</abstract><doi>10.48550/arxiv.2203.14915</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | DOI: 10.48550/arxiv.2203.14915 |
ispartof | |
issn | |
language | eng |
recordid | cdi_arxiv_primary_2203_14915 |
source | arXiv.org |
subjects | Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Physics - Experiment Physics - High Energy Physics - Phenomenology Physics - Instrumentation and Detectors Physics - Quantum Physics |
title | New Horizons: Scalar and Vector Ultralight Dark Matter |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T05%3A49%3A25IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=New%20Horizons:%20Scalar%20and%20Vector%20Ultralight%20Dark%20Matter&rft.au=Banerjee,%20A&rft.date=2022-03-28&rft_id=info:doi/10.48550/arxiv.2203.14915&rft_dat=%3Carxiv_GOX%3E2203_14915%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |