Soliton stars at finite temperature

Details Soliton stars at finite temperature Soliton stars at finite temperature

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44.1652c&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 44, Issue 6, 15 September 1991, pp.1652-1660

Physics

14

Scientific paper

We investigate the properties of soliton stars in the Lee-Wick model when a temperature dependence is introduced into this model. It is found that at some critical temperature Tc~100-200 MeV, a first-order phase transition occurs leading to the formation of soliton stars with characteristics similar to those considered by Lee and Pang but with a much smaller mass and size. We study the evolution of these soliton stars with the temperature from the early Universe to the present time.

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