New Horizons: Scalar and Vector Ultralight Dark Matter

New Horizons: Scalar and Vector Ultralight Dark Matter
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新视野：标量和矢量超轻暗物质

DOI：
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发表时间：
2022
期刊：
影响因子：
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通讯作者：
K. Zhou
K. Zhou
中科院分区：
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文献类型：
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作者：
D. Antypas;A. Banerjee;C. Bartram;M. Baryakhtar;J. Betz;J. Bollinger;C. Boutan;D. Bowring;D. Budker;D. Carney;G. Carosi;S. Chaudhuri;S. Cheong;A. Chou;M. D. Chowdhury;R. Co;José R. Crespo López;M. Demarteau;N. DePorzio;A. Derbin;T. Deshpande;L. Luzio;A. Díaz;J. Doyle;A. Drlica;A. Droster;N. Du;B. Dobrich;J. Eby;R. Essig;G. Farren;N. L. Figueroa;J. Fry;S. Gardner;A. Geraci;A. Ghalsasi;S. Ghosh;M. Giannotti;B. Gimeno;S. M. Griffin;D. Grin;H. Grote;J. Gundlach;M. Guzzetti;D. Hanneke;R. Harnik;R. Henning;V. Iršič;H. Jackson;D. F. Kimball;J. Jaeckel;M. Kagan;D. Kedar;R. Khatiwada;S. Knirck;S. Kolkowitz;T. Kovachy;S. Kuenstner;Z. Lasner;A. Leder;R. Lehnert;D. Leibrandt;E. Lentz;S. M. Lewis;Z. Liu;J. Manley;R. Maruyama;A. Millar;V. Muratova;Nathan Musoke;S. Nagaitsev;O. Noroozian;C. O’Hare;J. Ouellet;K. M. W. Pappas;E. Peik;G. Pérez;A. Phipps;N. Rapidis;J. Robinson;V. Robles;K. Rogers;J. Rudolph;G. Rybka;M. Safdari;M. Safronova;C. Salemi;P. O. Schmidt;T. Schumm;A. Schwartzman;J. Shu;M. Simanovskaia;J. Singh;S. Singh;M. S. Smith;W. Snow;Y. Stadnik;C. Sun;A. Sushkov;T. Tait;V. Takhistov;D. Tanner;D. Temples;P. Thirolf;J. Thomas;M. Tobar;O. Tretiak;Y. Tsai;J. Tyson;M. Vandegar;Sander M. Vermeulen;L. Visinelli;E. Vitagliano;Z. Wang;D. J. Wilson;L. Winslow;S. Withington;M. Wooten;J. Yang;J. Ye;B. Young;F. Yu;M. Zaheer;T. Zelevinsky;Y. Zhao;K. Zhou

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在过去的十年里，在所有质量尺度上建立暗物质模型方面做出了前所未有的努力，同时设计了许多新的探测策略。量子技术的革命性进步导致了大量新的高精度量子传感器和用于超轻($&lt；10\，$eV)玻色子暗物质的暗物质探测策略，这种物质可以用一个振荡的经典、基本上相干场来描述。这份白皮书的重点是寻找波状标量和矢量暗物质候选者。
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.