Gravitational stability of cold Bose star

E. Takasugi, M. Yoshimura

Research output: Contribution to journalArticlepeer-review

28 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/G3/2mN2 for the neutron star and may facilitate formation of smaller black holes made of cold invisible axions in the axion dominated universe.

Original languageEnglish
Pages (from-to)241-243
Number of pages3
JournalZeitschrift für Physik C Particles and Fields
Volume26
Issue number2
DOIs
Publication statusPublished - Jun 1 1984
Externally publishedYes

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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