Self-similar scalar soliton stars in the thin-wall approximation

Details Self-similar scalar soliton stars in the thin-wall approximation Self-similar scalar soliton stars in the thin-wall approximation

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44.2286d&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 44, Issue 8, 15 October 1991, pp.2286-2294

Physics

3

Scientific paper

Two families of time-dependent (analytical) solutions of Einstein equations, describing scalar soliton stars in the thin-wall approximation, are found and discussed. The space-time within the star is self-similar, reinforcing thereby the hypothesis about the formation of these objects during a second-order phase transition. Maximum and minimum values of the final surface potential, compatible with the asymptotic existence of the soliton star, are found.

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