On relativistic models of strange stars

Details On relativistic models of strange stars On relativistic models of strange stars

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007prama..68..397t&link_type=abstract

Pramana, vol. 68, Issue 3, p.397

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Relativistic Stellar Models, Superdense Stars, Strange

Scientific paper

The superdense stars with mass-to-size ratio exceeding 0.3 are expected to be made of strange matter. Assuming that the 3-space of the interior space--time of a strange star is that of a three-paraboloid immersed in a four-dimensional Euclidean space, we obtain a two-parameter family of their physically viable relativistic models. This ansatz determines density distribution of the interior self-gravitating matter up to one unknown parameter. The Einstein's field equations determine the fluid pressure and the remaining geometrical variables. The information about mass-to-size ratio together with the conventional boundary conditions lead to the determination of total mass, radius and other parameters of the stellar configuration.

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