English

Axion Dark Matter

High Energy Physics - Experiment 2023-03-31 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Instrumentation and Detectors

Abstract

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.

Keywords

Cite

@article{arxiv.2203.14923,
  title  = {Axion Dark Matter},
  author = {C. B. Adams and N. Aggarwal and A. Agrawal and R. Balafendiev and C. Bartram and M. Baryakhtar and H. Bekker and P. Belov and K. K. Berggren and A. Berlin and C. Boutan and D. Bowring and D. Budker and A. Caldwell and P. Carenza and G. Carosi and R. Cervantes and S. S. Chakrabarty and S. Chaudhuri and T. Y. Chen and S. Cheong and A. Chou and R. T. Co and J. Conrad and D. Croon and R. T. D'Agnolo and M. Demarteau and N. DePorzio and M. Descalle and K. Desch and L. Di Luzio and A. Diaz-Morcillo and K. Dona and I. S. Drachnev and A. Droster and N. Du and K. Dunne and B. Döbrich and S. A. R. Ellis and R. Essig and J. Fan and J. W. Foster and J. T. Fry and A. Gallo Rosso and J. M. García Barceló and I. G. Irastorza and S. Gardner and A. A. Geraci and S. Ghosh and B. Giaccone and M. Giannotti and B. Gimeno and D. Grin and H. Grote and M. Guzzetti and M. H. Awida and R. Henning and S. Hoof and G. Hoshino and V. Irsic and K. D. Irwin and H. Jackson and D. F. Jackson Kimball and J. Jaeckel and K. Jakovcic and M. J. Jewell and M. Kagan and Y. Kahn and R. Khatiwada and S. Knirck and T. Kovachy and P. Krueger and S. E. Kuenstner and N. A. Kurinsky and R. K. Leane and A. F. Leder and C. Lee and K. W. Lehnert and E. W. Lentz and S. M. Lewis and J. Liu and M. Lynn and B. Majorovits and D. J. E. Marsh and R. H. Maruyama and B. T. McAllister and A. J. Millar and D. W. Miller and J. Mitchell and S. Morampudi and G. Mueller and S. Nagaitsev and E. Nardi and O. Noroozian and C. A. J. O'Hare and N. S. Oblath and J. L. Ouellet and K. M. W. Pappas and H. V. Peiris and K. Perez and A. Phipps and M. J. Pivovaroff and P. Quílez and N. M. Rapidis and V. H. Robles and K. K. Rogers and J. Rudolph and J. Ruz and G. Rybka and M. Safdari and B. R. Safdi and M. S. Safronova and C. P. Salemi and P. Schuster and A. Schwartzman and J. Shu and M. Simanovskaia and J. Singh and S. Singh and K. Sinha and J. T. Sinnis and M. Siodlaczek and M. S. Smith and W. M. Snow and A. V. Sokolov and A. Sonnenschein and D. H. Speller and Y. V. Stadnik and C. Sun and A. O. Sushkov and T. M. P. Tait and V. Takhistov and D. B. Tanner and F. Tavecchio and D. J. Temples and J. H. Thomas and M. E. Tobar and N. Toro and Y. -D. Tsai and E. C. van Assendelft and K. van Bibber and M. Vandegar and L. Visinelli and E. Vitagliano and J. K. Vogel and Z. Wang and A. Wickenbrock and L. Winslow and S. Withington and M. Wooten and J. Yang and B. A. Young and F. Yu and K. Zhou and T. Zhou},
  journal= {arXiv preprint arXiv:2203.14923},
  year   = {2023}
}

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