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Relativistic Axions from Collapsing Bose Stars

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Levkov, D. G., Panin, A. G., Tkachev, I. I.·2017·Physical Review Letters

Abstract

The substructures of light bosonic (axionlike) dark matter may condense into compact Bose stars. We study the collapse of critical-mass stars caused by attractive self-interaction of the axionlike particles and find that these processes proceed in an unexpected universal way. First, nonlinear self-similar evolution (called "wave collapse" in condensed matter physics) forces the particles to fall into the star center. Second, interactions in the dense center create an outgoing stream of mildly relativistic particles which carries away an essential part of the star mass. The collapse stops when the star remnant is no longer able to support the self-similar infall feeding the collisions. We shortly discuss possible astrophysical and cosmological implications of these phenomena.

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Metadata

Authors
Levkov, D. G., Panin, A. G., & Tkachev, I. I.
Venue
Physical Review Letters
Published
2017-01-03
Volume
118
Issue
1
Pages
011301-011301
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2519167901
Cited by
167
References
0
FWCI
10.02
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Relativistic Axions from Collapsing Bose Stars. https://app.cochat.ai/papers/10.1103/physrevlett.118.011301
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Levkov, D. G., Panin, A. G., & Tkachev, I. I. (2017). Relativistic Axions from Collapsing Bose Stars. Physical Review Letters. https://doi.org/10.1103/physrevlett.118.011301

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