Thermalized Newtonian Bose Stars

Details Thermalized Newtonian Bose Stars Thermalized Newtonian Bose Stars

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.259..355d&link_type=abstract

Astrophysics and Space Science, v. 259, Issue 4, p. 355-369 (1998).

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We consider star models consisting of spin 0 particles interacting only gravitationally, e.g. Higgs-particles as possible dark matter objects. The particle gas of finite temperature is treated according to the Bose-Einstein-statistics in its non- relativistic limit; then the use of Newtonian gravity is sufficient too. The limits of these restrictions are estimated. The local temperature is determined with the use of energy conservation. The mass-radius relation of the objects and their further behaviours as Bose-Einstein-condensation in the outer regions are calculated. We find strong similarities with the features of white dwarfs and neutron stars.

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