2009/01/31 by P. Sikivie, Q. Yang, Qiaoli Yang · 10 citations
Physics and Astronomy · #Astrophysics #Axion #Cold Atom Physics and Bose-Einstein Condensates #Cold dark matter #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark fluid #Dark matter #Hot dark matter #Mixed dark matter #Particle physics #Physics #Scalar field dark matter #astro-ph.CO #cond-mat.stat-mech #hep-ph
paper · pdf · doi:10.1103/physrevlett.103.111301
published as Phys.Rev.Lett.103:111301,2009 · 4 pages. Three typos are corrected. Version to be published by Physical Review Letters
arxiv created 2009/09/02 · openalex publication_date 2009/09/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We show that cold dark matter axions thermalize and form a Bose-Einstein condensate (BEC). We obtain the axion state in a homogeneous and isotropic universe, and derive the equations governing small axion perturbations. Because they form a BEC, axions differ from ordinary cold dark matter in the nonlinear regime of structure formation and upon entering the horizon. Axion BEC provides a mechanism for the production of net overall rotation in dark matter halos, and for the alignment of cosmic microwave anisotropy multipoles.