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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: 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
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title
container_volume
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
fullrecord <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2203_14915</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2203_14915</sourcerecordid><originalsourceid>FETCH-LOGICAL-a675-a9678390b5d56be35f3079066f4c48cef3739e2fcae5645476b712633e54b4c73</originalsourceid><addsrcrecordid>eNotj8tOwzAQAH3pARU-gBP-gQQn613H3FB5FKktBwrXaOPaNCI0aGvx-npE4TS30YxSp5UpbYNozlk--_eyrg2UlfUVHilaxQ89H6X_Hnf7C_0QeGDRvNvopxjyKPpxyMJD_7zN-orlRS855yjHapJ42MeTf07V-uZ6PZsXi_vbu9nlomByWLAn14A3HW6QugiYwDhviJINtgkxgQMf6xQ4Ilm0jjpX1QQQ0XY2OJiqsz_tIbx9k_6V5av9HWgPA_ADYBo-wA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>New Horizons: Scalar and Vector Ultralight Dark Matter</title><source>arXiv.org</source><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</creator><creatorcontrib>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</creatorcontrib><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 ($&lt;10\,$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. D</creatorcontrib><creatorcontrib>Co, R. T</creatorcontrib><creatorcontrib>Demarteau, M</creatorcontrib><creatorcontrib>DePorzio, N</creatorcontrib><creatorcontrib>Derbin, A. V</creatorcontrib><creatorcontrib>Deshpande, T</creatorcontrib><creatorcontrib>Di Luzio, L</creatorcontrib><creatorcontrib>Diaz-Morcillo, A</creatorcontrib><creatorcontrib>Doyle, J. M</creatorcontrib><creatorcontrib>Drlica-Wagner, A</creatorcontrib><creatorcontrib>Droster, A</creatorcontrib><creatorcontrib>Du, N</creatorcontrib><creatorcontrib>Döbrich, B</creatorcontrib><creatorcontrib>Eby, J</creatorcontrib><creatorcontrib>Essig, R</creatorcontrib><creatorcontrib>Figueroa, N. L</creatorcontrib><creatorcontrib>Fry, J. T</creatorcontrib><creatorcontrib>Gardner, S</creatorcontrib><creatorcontrib>Geraci, A. A</creatorcontrib><creatorcontrib>Ghosh, S</creatorcontrib><creatorcontrib>Giannotti, M</creatorcontrib><creatorcontrib>Gimeno, B</creatorcontrib><creatorcontrib>Griffin, S. M</creatorcontrib><creatorcontrib>Grin, D</creatorcontrib><creatorcontrib>Grote, H</creatorcontrib><creatorcontrib>Gundlach, J. H</creatorcontrib><creatorcontrib>Guzzetti, M</creatorcontrib><creatorcontrib>Hanneke, D</creatorcontrib><creatorcontrib>Harnik, R</creatorcontrib><creatorcontrib>Henning, R</creatorcontrib><creatorcontrib>Irsic, V</creatorcontrib><creatorcontrib>Jackson, H</creatorcontrib><creatorcontrib>Kimball, D. F. Jackson</creatorcontrib><creatorcontrib>Jaeckel, J</creatorcontrib><creatorcontrib>Kagan, M</creatorcontrib><creatorcontrib>Khatiwada, R</creatorcontrib><creatorcontrib>Knirck, S</creatorcontrib><creatorcontrib>Kovachy, T</creatorcontrib><creatorcontrib>Kuenstner, S. E</creatorcontrib><creatorcontrib>Lasner, Z</creatorcontrib><creatorcontrib>Leder, A. F</creatorcontrib><creatorcontrib>Lehnert, R</creatorcontrib><creatorcontrib>Leibrandt, D. R</creatorcontrib><creatorcontrib>Lewis, S. M</creatorcontrib><creatorcontrib>Manley, J</creatorcontrib><creatorcontrib>Maruyama, R. H</creatorcontrib><creatorcontrib>Muratova, V. N</creatorcontrib><creatorcontrib>O'Hare, C. A. J</creatorcontrib><creatorcontrib>Ouellet, J. L</creatorcontrib><creatorcontrib>Pappas, K. M. W</creatorcontrib><creatorcontrib>Peik, E</creatorcontrib><creatorcontrib>Perez, G</creatorcontrib><creatorcontrib>Robles, V. H</creatorcontrib><creatorcontrib>Safdari, M</creatorcontrib><creatorcontrib>Safronova, M. S</creatorcontrib><creatorcontrib>Salemi, C. P</creatorcontrib><creatorcontrib>Schmidt, P. O</creatorcontrib><creatorcontrib>Schumm, T</creatorcontrib><creatorcontrib>Schwartzman, A</creatorcontrib><creatorcontrib>Shu, J</creatorcontrib><creatorcontrib>Simanovskaia, M</creatorcontrib><creatorcontrib>Smith, M. S</creatorcontrib><creatorcontrib>Snow, W. M</creatorcontrib><creatorcontrib>Stadnik, Y. V</creatorcontrib><creatorcontrib>Sun, C</creatorcontrib><creatorcontrib>Sushkov, A. 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><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 ($&lt;10\,$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. D</creator><creator>Co, R. T</creator><creator>Demarteau, M</creator><creator>DePorzio, N</creator><creator>Derbin, A. V</creator><creator>Deshpande, T</creator><creator>Di Luzio, L</creator><creator>Diaz-Morcillo, A</creator><creator>Doyle, J. M</creator><creator>Drlica-Wagner, A</creator><creator>Droster, A</creator><creator>Du, N</creator><creator>Döbrich, B</creator><creator>Eby, J</creator><creator>Essig, R</creator><creator>Figueroa, N. L</creator><creator>Fry, J. T</creator><creator>Gardner, S</creator><creator>Geraci, A. A</creator><creator>Ghosh, S</creator><creator>Giannotti, M</creator><creator>Gimeno, B</creator><creator>Griffin, S. M</creator><creator>Grin, D</creator><creator>Grote, H</creator><creator>Gundlach, J. H</creator><creator>Guzzetti, M</creator><creator>Hanneke, D</creator><creator>Harnik, R</creator><creator>Henning, R</creator><creator>Irsic, V</creator><creator>Jackson, H</creator><creator>Kimball, D. F. Jackson</creator><creator>Jaeckel, J</creator><creator>Kagan, M</creator><creator>Khatiwada, R</creator><creator>Knirck, S</creator><creator>Kovachy, T</creator><creator>Kuenstner, S. E</creator><creator>Lasner, Z</creator><creator>Leder, A. F</creator><creator>Lehnert, R</creator><creator>Leibrandt, D. R</creator><creator>Lewis, S. M</creator><creator>Manley, J</creator><creator>Maruyama, R. H</creator><creator>Muratova, V. N</creator><creator>O'Hare, C. A. J</creator><creator>Ouellet, J. L</creator><creator>Pappas, K. M. W</creator><creator>Peik, E</creator><creator>Perez, G</creator><creator>Robles, V. H</creator><creator>Safdari, M</creator><creator>Safronova, M. S</creator><creator>Salemi, C. P</creator><creator>Schmidt, P. O</creator><creator>Schumm, T</creator><creator>Schwartzman, A</creator><creator>Shu, J</creator><creator>Simanovskaia, M</creator><creator>Smith, M. S</creator><creator>Snow, W. M</creator><creator>Stadnik, Y. V</creator><creator>Sun, C</creator><creator>Sushkov, A. O</creator><creator>Tait, T. M. P</creator><creator>Takhistov, V</creator><creator>Tanner, D. B</creator><creator>Temples, D. J</creator><creator>Thomas, J. H</creator><creator>Tobar, M. E</creator><creator>Tretiak, O</creator><creator>Tsai, Y. -D</creator><creator>Tyson, J. A</creator><creator>Vandegar, M</creator><creator>Vermeulen, S</creator><creator>Visinelli, L</creator><creator>Wang, Z</creator><creator>Wilson, D. J</creator><creator>Winslow, L</creator><creator>Withington, S</creator><creator>Yang, J</creator><creator>Ye, J</creator><creator>Young, B. A</creator><creator>Yu, F</creator><creator>Zaheer, M. 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. H ; Zelevinsky, T ; Zhao, Y ; Zhou, K</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a675-a9678390b5d56be35f3079066f4c48cef3739e2fcae5645476b712633e54b4c73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Physics - Instrumentation and Detectors</topic><topic>Physics - Quantum Physics</topic><toplevel>online_resources</toplevel><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. D</creatorcontrib><creatorcontrib>Co, R. T</creatorcontrib><creatorcontrib>Demarteau, M</creatorcontrib><creatorcontrib>DePorzio, N</creatorcontrib><creatorcontrib>Derbin, A. V</creatorcontrib><creatorcontrib>Deshpande, T</creatorcontrib><creatorcontrib>Di Luzio, L</creatorcontrib><creatorcontrib>Diaz-Morcillo, A</creatorcontrib><creatorcontrib>Doyle, J. M</creatorcontrib><creatorcontrib>Drlica-Wagner, A</creatorcontrib><creatorcontrib>Droster, A</creatorcontrib><creatorcontrib>Du, N</creatorcontrib><creatorcontrib>Döbrich, B</creatorcontrib><creatorcontrib>Eby, J</creatorcontrib><creatorcontrib>Essig, R</creatorcontrib><creatorcontrib>Figueroa, N. L</creatorcontrib><creatorcontrib>Fry, J. T</creatorcontrib><creatorcontrib>Gardner, S</creatorcontrib><creatorcontrib>Geraci, A. A</creatorcontrib><creatorcontrib>Ghosh, S</creatorcontrib><creatorcontrib>Giannotti, M</creatorcontrib><creatorcontrib>Gimeno, B</creatorcontrib><creatorcontrib>Griffin, S. M</creatorcontrib><creatorcontrib>Grin, D</creatorcontrib><creatorcontrib>Grote, H</creatorcontrib><creatorcontrib>Gundlach, J. H</creatorcontrib><creatorcontrib>Guzzetti, M</creatorcontrib><creatorcontrib>Hanneke, D</creatorcontrib><creatorcontrib>Harnik, R</creatorcontrib><creatorcontrib>Henning, R</creatorcontrib><creatorcontrib>Irsic, V</creatorcontrib><creatorcontrib>Jackson, H</creatorcontrib><creatorcontrib>Kimball, D. F. Jackson</creatorcontrib><creatorcontrib>Jaeckel, J</creatorcontrib><creatorcontrib>Kagan, M</creatorcontrib><creatorcontrib>Khatiwada, R</creatorcontrib><creatorcontrib>Knirck, S</creatorcontrib><creatorcontrib>Kovachy, T</creatorcontrib><creatorcontrib>Kuenstner, S. E</creatorcontrib><creatorcontrib>Lasner, Z</creatorcontrib><creatorcontrib>Leder, A. F</creatorcontrib><creatorcontrib>Lehnert, R</creatorcontrib><creatorcontrib>Leibrandt, D. R</creatorcontrib><creatorcontrib>Lewis, S. M</creatorcontrib><creatorcontrib>Manley, J</creatorcontrib><creatorcontrib>Maruyama, R. H</creatorcontrib><creatorcontrib>Muratova, V. N</creatorcontrib><creatorcontrib>O'Hare, C. A. J</creatorcontrib><creatorcontrib>Ouellet, J. L</creatorcontrib><creatorcontrib>Pappas, K. M. W</creatorcontrib><creatorcontrib>Peik, E</creatorcontrib><creatorcontrib>Perez, G</creatorcontrib><creatorcontrib>Robles, V. H</creatorcontrib><creatorcontrib>Safdari, M</creatorcontrib><creatorcontrib>Safronova, M. S</creatorcontrib><creatorcontrib>Salemi, C. P</creatorcontrib><creatorcontrib>Schmidt, P. O</creatorcontrib><creatorcontrib>Schumm, T</creatorcontrib><creatorcontrib>Schwartzman, A</creatorcontrib><creatorcontrib>Shu, J</creatorcontrib><creatorcontrib>Simanovskaia, M</creatorcontrib><creatorcontrib>Smith, M. S</creatorcontrib><creatorcontrib>Snow, W. M</creatorcontrib><creatorcontrib>Stadnik, Y. V</creatorcontrib><creatorcontrib>Sun, C</creatorcontrib><creatorcontrib>Sushkov, A. 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 ($&lt;10\,$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