On the stability of tension stars

Details On the stability of tension stars On the stability of tension stars

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.255..379b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, April 1, 1992, p. 379-381.

Astronomy and Astrophysics

Astronomy

1

Einstein Equations, Equilibrium Equations, Stellar Envelopes, Stellar Motions, Equations Of Motion, Numerical Stability, Star Formation

Scientific paper

False vacuum material has been invoked to drive an inflationary phase in the very early universe, which leads to the belief that relics of the false vacuum may exist today. It was recently suggested that stars composed of such material, encased in a shell of ordinary matter, may have survived to the present era. The mechanically stability of the proposed solutions of Einstein's field equations is examined, and it is shown that stable equilibrium configurations consistent with the dominant energy condition are only possible for certain values of the parameters.

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