CERN Accélérateur de science

Preprint
Report number	arXiv:2203.14923 ; FERMILAB-CONF-22-996-PPD-T
Title	Axion Dark Matter
Author(s)	Adams, C.B. (Columbia U.) ; Aggarwal, N. ; Agrawal, A. (Chicago U.) ; Balafendiev, R. (ITMO U., St. Petersburg) ; Bartram, C. (Washington U., Seattle) ; Baryakhtar, M. (Washington U., Seattle) ; Bekker, H. (Helmholtz Inst., Mainz ; Mainz U.) ; Belov, P. (ITMO U., St. Petersburg) ; Berggren, K.K. (MIT) ; Berlin, A. (Fermilab) ; Boutan, C. (PNL, Richland) ; Bowring, D. (Fermilab) ; Budker, D. (Helmholtz Inst., Mainz ; Mainz U. ; UC, Berkeley) ; Caldwell, A. ; Carenza, P. ; Carosi, G. (LLNL, Livermore ; Washington U., Seattle) ; Cervantes, R. ; Chakrabarty, S.S. (INFN, Turin) ; Chaudhuri, S. (Princeton U.) ; Chen, T.Y. ; Cheong, S. (SLAC ; Stanford U., Phys. Dept.) ; Chou, A. (Fermilab) ; Co, R.T. (Minnesota U., Theor. Phys. Inst.) ; Conrad, J. (Stockholm U., OKC) ; Croon, D. ; D'Agnolo, R.T. (IPhT, Saclay ; Bohr Inst.) ; Demarteau, M. (Oak Ridge) ; DePorzio, N. (Harvard-Smithsonian Ctr. Astrophys.) ; Descalle, M. ; Desch, K. ; Di Luzio, L. (U. Padua, Dept. Phys. Astron. ; INFN, Padua) ; Diaz-Morcillo, A. (Cartagena Politecnica U.) ; Dona, K. ; Drachnev, I.S. ; Droster, A. (UC, Berkeley) ; Du, N. (LLNL, Livermore) ; Dunne, K. (Stockholm U., OKC) ; Döbrich, B. (CERN) ; Ellis, S.A.R. (Geneva U., Dept. Theor. Phys.) ; Essig, R. (YITP, Stony Brook) ; Fan, J. (Brown U.) ; Foster, J.W. (MIT, Cambridge, CTP) ; Fry, J.T. (MIT, LNS) ; Gallo Rosso, A. (Stockholm U., OKC) ; Barceló, J.M. García (Cartagena Politecnica U.) ; Irastorza, I.G. (Zaragoza U.) ; Gardner, S. (Kentucky U.) ; Geraci, A.A. (Northwestern U.) ; Ghosh, S. (Yale U.) ; Giaccone, B. ; Giannotti, M. (Barry U.) ; Gimeno, B. (Valencia U., IFIC) ; Grin, D. (Haverford Coll.) ; Grote, H. (Cardiff U.) ; Guzzetti, M. (Washington U., Seattle) ; Awida, M.H. (Fermilab) ; Henning, R. (North Carolina U. ; Duke U. ; TUNL, Durham) ; Hoof, S. (Inst. Astrophys. Gottingen) ; Hoshino, G. ; Irsic, V. (Cambridge U.) ; Irwin, K.D. ; Jackson, H. (UC, Berkeley) ; Kimball, D.F. Jackson (Cal State, East Bay) ; Jaeckel, J. (Heidelberg U.) ; Jakovcic, K. ; Jewell, M.J. ; Kagan, M. (SLAC) ; Kahn, Y. (Illinois U., Urbana (main)) ; Khatiwada, R. (Fermilab ; IIT, Chicago) ; Knirck, S. (Fermilab) ; Kovachy, T. (Northwestern U.) ; Krueger, P. (Braunschweig, Phys. Tech. Bund.) ; Kuenstner, S.E. (Stanford U., Phys. Dept.) ; Kurinsky, N.A. (SLAC ; KIPAC, Menlo Park) ; Leane, R.K. (SLAC ; KIPAC, Menlo Park) ; Leder, A.F. (UC, Berkeley ; LBL, Berkeley) ; Lee, C. (Munich, Max Planck Inst.) ; Lehnert, K.W. (JILA, Boulder ; NIST, Boulder ; Colorado U.) ; Lentz, E.W. (PNL, Richland) ; Lewis, S.M. (Fermilab) ; Liu, J. (Cambridge U.) ; Lynn, M. (Chicago U.) ; Majorovits, B. (Heidelberg, Max Planck Inst.) ; Marsh, D.J.E. (King's Coll. London) ; Maruyama, R.H. (Yale U.) ; McAllister, B.T. (Western Australia U. ; Swinburne U. Tech., Hawthorn) ; Millar, A.J. (Stockholm U., OKC ; Nordita ; Royal Inst. Tech., Stockholm) ; Miller, D.W. (Chicago U.) ; Mitchell, J. ; Morampudi, S. (MIT, Cambridge, CTP) ; Mueller, G. (U. Florida, Gainesville (main)) ; Nagaitsev, S. (Fermilab ; Chicago U.) ; Nardi, E. ; Noroozian, O. (NASA, Houston) ; O'Hare, C.A.J. (Sydney U.) ; Oblath, N.S. (PNL, Richland) ; Ouellet, J.L. (MIT, LNS) ; Pappas, K.M.W. (MIT, LNS) ; Peiris, H.V. (Stockholm U., OKC) ; Perez, K. (MIT, LNS) ; Phipps, A. (Cal State, East Bay) ; Pivovaroff, M.J. (LLNL, Livermore) ; Quílez, P. (DESY) ; Rapidis, N.M. (Stanford U., Phys. Dept.) ; Robles, V.H. (Yale Ctr. Astron. Astrophys.) ; Rogers, K.K. (Canadian Inst. Theor. Astrophys.) ; Rudolph, J. (Stanford U., Phys. Dept.) ; Ruz, J. (Zaragoza U.) ; Rybka, G. (Washington U., Seattle) ; Safdari, M. (SLAC ; Stanford U., Phys. Dept.) ; Safdi, B.R. (UC, Berkeley) ; Safronova, M.S. (Delaware U.) ; Salemi, C.P. (MIT, LNS) ; Schuster, P. (SLAC) ; Schwartzman, A. (SLAC) ; Shu, J. (Beijing, Inst. Theor. Phys.) ; Simanovskaia, M. (Stanford U., Phys. Dept.) ; Singh, J. (Stanford U., Phys. Dept.) ; Singh, S. (U. Delaware, Newark ; Delaware U.) ; Sinha, K. (Oklahoma U.) ; Sinnis, J.T. (Washington U., Seattle) ; Siodlaczek, M. (CERN) ; Smith, M.S. (Oak Ridge) ; Snow, W.M. (Indiana U.) ; Sokolov, A.V. (DESY) ; Sonnenschein, A. (Fermilab) ; Speller, D.H. (Johns Hopkins U.) ; Stadnik, Y.V. (Sydney U.) ; Sun, C. (Tel Aviv U.) ; Sushkov, A.O. (Boston U.) ; Tait, T.M.P. (UC, Irvine) ; Takhistov, V. (Tokyo U., IPMU) ; Tanner, D.B. (U. Florida, Gainesville (main)) ; Tavecchio, F. ; Temples, D.J. (Fermilab) ; Thomas, J.H. (IIT, Chicago) ; Tobar, M.E. (Western Australia U.) ; Toro, N. (SLAC) ; Tsai, Y.-D. (UC, Irvine ; Fermilab) ; van Assendelft, E.C. ; van Bibber, K. (UC, Berkeley) ; Vandegar, M. (SLAC) ; Visinelli, L. (Tsung-Dao Lee Inst., Shanghai ; Shanghai Jiaotong U.) ; Vitagliano, E. (UCLA) ; Vogel, J.K. (Zaragoza U. ; LLNL, Livermore) ; Wang, Z. (New York U., CCPP) ; Wickenbrock, A. (Mainz U. ; Helmholtz Inst., Mainz) ; Winslow, L. (MIT, LNS) ; Withington, S. (Cambridge U.) ; Wooten, M. (UC, Berkeley) ; Yang, J. (PNL, Richland) ; Young, B.A. (Haimson Res., Santa Clara) ; Yu, F. (U. Mainz, PRISMA) ; Zhou, K. (SLAC) ; Zhou, T. (MIT)
Imprint	2022-03-28
Number of pages	96
Note	restore and expand author list
Presented at	2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.
Subject category	physics.ins-det ; Detectors and Experimental Techniques ; hep-ph ; Particle Physics - Phenomenology ; astro-ph.CO ; Astrophysics and Astronomy ; hep-ex ; Particle Physics - Experiment
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.
Other source	Inspire
Copyright/License	preprint: (License: CC BY 4.0)