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Preprint
Report number arXiv:2203.14915 ; FERMILAB-PUB-22-262-AD-PPD-T
Title New Horizons: Scalar and Vector Ultralight Dark Matter
Related titleNew Horizons: Scalar and Vector Ultralight Dark Matter
Author(s) Antypas, D. (Mainz U. ; Helmholtz Inst., Mainz) ; Banerjee, A. (Weizmann Inst.) ; Bartram, C. (Washington U., Seattle) ; Baryakhtar, M. (Washington U., Seattle) ; Betz, J. (U. Delaware, Newark) ; Bollinger, J.J. (NIST, Boulder) ; Boutan, C. (PNL, Richland) ; Bowring, D. (Fermilab) ; Budker, D. (Helmholtz Inst., Mainz ; Mainz U. ; UC, Berkeley) ; Carney, D. (LBL, Berkeley) ; Carosi, G. (LLNL, Livermore ; Washington U., Seattle) ; Chaudhuri, S. (Princeton U.) ; Cheong, S. (SLAC ; Stanford U., Phys. Dept.) ; Chou, A. (Fermilab) ; Chowdhury, M.D. (Arizona U., Optical Sci. Ctr.) ; Co, R.T. (Minnesota U., Theor. Phys. Inst.) ; Crespo López-Urrutia, J.R. (Heidelberg, Max Planck Inst.) ; Demarteau, M. (Oak Ridge) ; DePorzio, N. (Harvard U.) ; Derbin, A.V. (St. Petersburg, INP) ; Deshpande, T. (Northwestern U.) ; Chowdhury, M.D. (Helmholtz Inst., Mainz ; Arizona U., Optical Sci. Ctr.) ; Di Luzio, L. (U. Padua, Dept. Phys. Astron. ; INFN, Padua) ; Diaz-Morcillo, A. (Cartagena Politecnica U.) ; Doyle, J.M. (Harvard U.) ; Drlica-Wagner, A. (Fermilab ; Chicago U., KICP ; Chicago U.) ; Droster, A. (UC, Berkeley) ; Du, N. (LLNL, Livermore) ; Döbrich, B. (CERN) ; Eby, J. (Tokyo U., IPMU) ; Essig, R. (YITP, Stony Brook) ; Farren, G.S. (Cambridge U., DAMTP) ; Figueroa, N.L. (Mainz U. ; Helmholtz Inst., Mainz) ; Fry, J.T. (MIT, LNS) ; Gardner, S. (Kentucky U.) ; Geraci, A.A. (Northwestern U.) ; Ghalsasi, A. (Pittsburgh U.) ; Ghosh, S. (Yale U.) ; Giannotti, M. (Barry U.) ; Gimeno, B. (Valencia U., IFIC) ; Griffin, S.M. (LBNL, NSD ; LBL, Berkeley) ; Grin, D. (Haverford Coll.) ; Grin, D. (Helmholtz Inst., Mainz ; Haverford Coll.) ; Grote, H. (Cardiff U.) ; Gundlach, J.H. (Washington U., Seattle) ; Guzzetti, M. (Washington U., Seattle) ; Hanneke, D. (Amherst Coll.) ; Harnik, R. (Fermilab) ; Henning, R. (North Carolina U. ; Duke U. ; TUNL, Durham) ; Irsic, V. (Cambridge U.) ; Jackson, H. (UC, Berkeley) ; Kimball, D.F. Jackson (Cal State, East Bay) ; Jaeckel, J. (Heidelberg U.) ; Kagan, M. (SLAC) ; Kedar, D. (JILA, Boulder ; Colorado U.) ; Khatiwada, R. (Fermilab ; IIT, Chicago) ; Knirck, S. (Fermilab) ; Kolkowitz, S. (Wisconsin U., Madison) ; Kovachy, T. (Northwestern U.) ; Kuenstner, S.E. (Stanford U., Phys. Dept.) ; Lasner, Z. (Harvard U.) ; Leder, A.F. (UC, Berkeley ; LBL, Berkeley) ; Lehnert, R. (Indiana U., Bloomington (main)) ; Leibrandt, D.R. (NIST, Boulder ; Colorado U.) ; Lentz, E. (PNL, Richland) ; Lewis, S.M. (Fermilab) ; Liu, Z. (Minnesota U.) ; Manley, J. (Delaware U.) ; Maruyama, R.H. (Yale U.) ; Millar, A.J. (Stockholm U., OKC ; Nordita ; Royal Inst. Tech., Stockholm) ; Muratova, V.N. (St. Petersburg, INP) ; Musoke, N. (New Hampshire U.) ; Nagaitsev, S. (Fermilab ; Chicago U.) ; Noroozian, O. (NASA, Houston) ; O'Hare, C.A.J. (Sydney U.) ; Ouellet, J.L. (MIT, LNS) ; Pappas, K.M.W. (MIT, LNS) ; Peik, E. (Braunschweig, Phys. Tech. Bund.) ; Perez, G. (Weizmann Inst.) ; Phipps, A. (Cal State, East Bay) ; Rapidis, N.M. (Stanford U., Phys. Dept.) ; Robinson, J.M. (JILA, Boulder ; Colorado U.) ; Robles, V.H. (Yale Ctr. Astron. Astrophys.) ; Rogers, K.K. (Canadian Inst. Theor. Astrophys.) ; Rudolph, J. (Stanford U., Phys. Dept.) ; Rybka, G. (Washington U., Seattle) ; Safdari, M. (SLAC ; Stanford U., Phys. Dept.) ; Safdari, M. (Helmholtz Inst., Mainz ; Stanford U., Phys. Dept. ; SLAC) ; Safronova, M.S. (Delaware U., Bartol Inst.) ; Salemi, C.P. (MIT, LNS) ; Schmidt, P.O. (Braunschweig, Phys. Tech. Bund. ; Hannover U.) ; Schumm, T. (Vienna, Tech. U., Atominst.) ; Schwartzman, A. (SLAC) ; Shu, J. (Beijing, Inst. Theor. Phys.) ; Simanovskaia, M. (Stanford U., Phys. Dept.) ; Singh, J. (Stanford U., Phys. Dept.) ; Singh, S. (Delaware U. ; Delaware U., Bartol Inst.) ; Smith, M.S. (Oak Ridge) ; Snow, W.M. (Indiana U., Bloomington (main)) ; 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)) ; Temples, D.J. (Fermilab) ; Thirolf, P.G. (Munich U.) ; Thomas, J.H. (IIT, Chicago) ; Tobar, M.E. (Western Australia U.) ; Tretiak, O. (Mainz U. ; Helmholtz Inst., Mainz) ; Tsai, Y.-D. (UC, Irvine ; Fermilab) ; Tyson, J.A. (LLNL, Livermore ; UC, Davis) ; Vandegar, M. (SLAC) ; Vermeulen, S. (Cardiff U.) ; Visinelli, L. (Tsung-Dao Lee Inst., Shanghai ; Shanghai Jiaotong U.) ; Vitagliano, E. (UCLA) ; Wang, Z. (New York U., CCPP) ; Wilson, D.J. (Arizona U., Optical Sci. Ctr.) ; Winslow, L. (MIT, LNS) ; Withington, S. (Cambridge U.) ; Wooten, M. (UC, Berkeley) ; Yang, J. (PNL, Richland) ; Ye, J. (JILA, Boulder ; Colorado U.) ; Young, B.A. (Haimson Res., Santa Clara) ; Yu, F. (U. Mainz, PRISMA) ; Zaheer, M.H. (Delaware U., Bartol Inst.) ; Zelevinsky, T. (Munich, Max Planck Inst. ; Columbia U.) ; Zhao, Y. (Utah U.) ; Zhou, K. (SLAC)
Imprint 2022-03-28
Number of pages 89
Note Snowmass 2021 White Paper
Presented at 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.
Subject category quant-ph ; General Theoretical Physics ; physics.ins-det ; Detectors and Experimental Techniques ; hep-ph ; Particle Physics - Phenomenology ; astro-ph.CO ; Astrophysics and Astronomy ; hep-ex ; Particle Physics - Experiment
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 ($<10\,$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.
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Copyright/License preprint: (License: arXiv nonexclusive-distrib 1.0)

10^{-23}\,\mathrm{eV}\) for UDM being all the DM \cite{2021arXiv211101199D}. The strongest bound from the Lyman-alpha forest (Ly\(\alpha\)f) sets \(m_\phi > 2 \times 10^{-20}\,\mathrm{eV}\) for UDM being all the DM \cite{2021PhRvL.126g1302R}, while \cite{Kobayashi:2017jcf} considered a sub-dominant contribution to the DM. UDM is also excluded from galaxy rotation curves in the SPARC database \cite{Bar:2021kti}; a combination of the high-redshift UV luminosity function and the optical depth to reionization (Rei.) \cite{Bozek:2014uqa}; and the Milky Way sub-halo mass function (MW) \cite{Nadler200800022}. The central star cluster in the dwarf galaxy Eridanus-II (Eri.-II) can be used to exclude \(m_\phi \sim 10^{-20}\,\mathrm{eV}\) \cite{2019PhRvL.123e1103M}, while black hole superradiance (BHSR) probes \(m_\phi \sim 10^{-18}\,\mathrm{eV}\) (although there are differences between analyses) \cite{Arvanitaki:2010sy,Arvanitaki:2014wva,Brito:2014wla,Brito:2015oca,Arvanitaki:2016qwi,Brito:2017zvb,Cardoso:2018tly,Caputo:2021efm}. Pulsar timing array (PTA) residuals are sensitive to gravitational potential oscillations for \(m_\phi \sim 10^{-23}\,\mathrm{eV}\). A future intensity mapping survey from the Square Kilometre Array (SKA-IM) could probe up to \(m_\phi \sim 10^{-22}\,\mathrm{eV}\) and \(\Omega_\phi \sim 10^{-4}\). For \(m_\phi < 10^{-30}\,\mathrm{eV}\), the ultralight scalars behave like dark energy and do not contribute to the dark matter density." width="200px"/> Show more plots


 


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