Abstract
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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.