Gravitational stability of cold Bose star

Details Gravitational stability of cold Bose star Gravitational stability of cold Bose star

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984zphyc..26..241t&link_type=abstract

Zeitschrift für Physik C Particles and Fields, Volume 26, Issue 2, pp.241-243

Physics

12

Scientific paper

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 3/2 m {/N 2} for the neutron star and may facilitate formation of smaller black holes made of cold invisible axions in the axion dominated universe.

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