Gravitational stability of cold Bose star

E. Takasugi; M. Yoshimura

doi:10.1007/BF01421759

Gravitational stability of cold Bose star

E. Takasugi, M. Yoshimura

研究成果 › 査読

31 被引用数 (Scopus)

抄録

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.

本文言語	English
ページ（範囲）	241-243
ページ数	3
ジャーナル	Zeitschrift für Physik C Particles and Fields
巻	26
号	2
DOI	https://doi.org/10.1007/BF01421759
出版ステータス	Published - 6月 1 1984
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（その他）

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10.1007/BF01421759

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Gravitational stability of cold Bose star

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