Axion Dark Matter

C. B. Adams, N. Aggarwal, A. Agrawal,R. Balafendiev,C. Bartram,M. Baryakhtar,H. Bekker,P. Belov,K. K. Berggren, A. Berlin,C. Boutan, D. Bowring, D. Budker, A. Caldwell, P. Carenza,G. Carosi, R. Cervantes,S. S. Chakrabarty,S. Chaudhuri, T. Y. Chen,S. Cheong,A. Chou,R. T. Co,J. Conrad, D. Croon, R. T. D'Agnolo,M. Demarteau,N. DePorzio, M. Descalle, K. Desch,L. Di Luzio,A. Diaz-Morcillo, K. Dona, I. S. Drachnev,A. Droster,N. Du, K. Dunne, B. Döbrich,S. A. R. Ellis, R. Essig, J. Fan,J. W. Foster,J. T. Fry, A. Gallo Rosso, J. M. García Barceló,I. G. Irastorza,S. Gardner,A. A. Geraci,S. Ghosh, B. Giaccone,M. Giannotti, B. Gimeno, D. Grin,H. Grote,M. Guzzetti,M. H. Awida,R. Henning,S. Hoof, G. Hoshino,V. Irsic,K. D. Irwin, H. Jackson,D. F. Jackson Kimball, J. Jaeckel, K. Jakovcic, M. J. Jewell, M. Kagan,Y. Kahn,R. Khatiwada,S. Knirck,T. Kovachy, P. Krueger,S. E. Kuenstner,N. A. Kurinsky,R. K. Leane,A. F. Leder,C. Lee,K. W. Lehnert,E. W. Lentz,S. M. Lewis, J. Liu, M. Lynn, B. Majorovits,D. J. E. Marsh,R. H. Maruyama,B. T. McAllister, A. J. Millar,D. W. Miller, J. Mitchell,S. Morampudi,G. Mueller, S. Nagaitsev,E. Nardi,O. Noroozian,C. A. J. O'Hare,N. S. Oblath,J. L. Ouellet, K. M. W. Pappas,H. V. Peiris,K. Perez,A. Phipps,M. J. Pivovaroff, P. Quílez,N. M. Rapidis, V. H. Robles,K. K. Rogers,J. Rudolph,J. Ruz, G. Rybka,M. Safdari,B. R. Safdi,M. S. Safronova,C. P. Salemi, P. Schuster, A. Schwartzman,J. Shu, M. Simanovskaia,J. Singh,S. Singh,K. Sinha, J. T. Sinnis, M. Siodlaczek,M. S. Smith,W. M. Snow, A. V. Sokolov,A. Sonnenschein,D. H. Speller,Y. V. Stadnik, C. Sun,A. O. Sushkov,T. M. P. Tait, V. Takhistov, D. B. Tanner, F. Tavecchio, D. J. Temples,J. H. Thomas,M. E. Tobar, N. Toro,Y. -D. Tsai, E. C. van Assendelft,K. van Bibber,M. Vandegar,L. Visinelli,E. Vitagliano,J. K. Vogel,Z. Wang,A. Wickenbrock,L. Winslow, S. Withington, M. Wooten, J. Yang,B. A. Young,F. Yu,K. Zhou,T. Zhou

arxiv（2023）

引用 1|浏览41

暂无评分

摘要

Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white paper summarizes axion phenomenology and outlines next-generation laboratory experiments proposed to detect axion dark matter. There are vibrant synergies with astrophysical searches and advances in instrumentation including quantum-enabled readout, high-Q resonators and cavities and large high-field magnets. This white paper outlines a clear roadmap to discovery, and shows that the US is well-positioned to be at the forefront of the search for axion dark matter in the coming decade.

查看译文

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要