Gravitational stability of cold Bose star

E. Takasugi; M. Yoshimura

doi:10.1007/BF01421759

Gravitational stability of cold Bose star

E. Takasugi, M. Yoshimura

Research output: Contribution to journal › Article › peer-review

33 Citations (Scopus)

Abstract

The maximum mass of cold Bose star that can sustain its own gravity is determined to be ≈0.6/Gm, where m is the mass of boson. This is different from the Oppenheimer-Volkoff mass of ≈0.4/G^3/2m_N² for the neutron star and may facilitate formation of smaller black holes made of cold invisible axions in the axion dominated universe.

Original language	English
Pages (from-to)	241-243
Number of pages	3
Journal	Zeitschrift für Physik C Particles and Fields
Volume	26
Issue number	2
DOIs	https://doi.org/10.1007/BF01421759
Publication status	Published - Jun 1 1984
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1007/BF01421759

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Gravitational stability of cold Bose star

Abstract

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