Structure of the self-gravitating dilute-boson sphere

Details Structure of the self-gravitating dilute-boson sphere Structure of the self-gravitating dilute-boson sphere

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...241....1m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 1, Jan. 1991, p. 1-4. Research supported by DGICYT.

Statistics

Computation

25

Bosons, Dark Matter, Gravitational Effects, Computational Astrophysics, Cosmochemistry, Particle Density (Concentration), Carbon Isotopic Ratio, Stars: Abundances, Stars: Carbon, Stars: Ch, Stars: Population Ii

Scientific paper

The sensitivity of the Newtonian self-gravitating dilute-boson-gas solution obtained by Membrado et al. (1989) and Abad et al. (1989) is investigated analytically. Particular attention is given to the effects of (1) including the second leading term in the equation of state and (2) introducing a repulsive cosmological constant. The derivation is outlined; the general trends are shown in graphs; and the case of the axion is treated as an example.

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