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Bose-Einstein Condensation of Dark Matter Axions

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Sikivie, P., Yang, Q.·2009·Physical Review Letters

Abstract

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.

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Metadata

Authors
Sikivie, P., & Yang, Q.
Venue
Physical Review Letters
Published
2009-09-09
Volume
103
Issue
11
Pages
111301-111301
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2070455023
Cited by
475
References
0
FWCI
9.89
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Bose-Einstein Condensation of Dark Matter Axions. https://app.cochat.ai/papers/10.1103/physrevlett.103.111301
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Sikivie, P., & Yang, Q. (2009). Bose-Einstein Condensation of Dark Matter Axions. Physical Review Letters. https://doi.org/10.1103/physrevlett.103.111301

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.