Spherically symmetric models for stars and voids II: constraints on the radial pressures

Details Spherically symmetric models for stars and voids II: constraints on the radial pressures Spherically symmetric models for stars and voids II: constraints on the radial pressures

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21.1351f&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 6, pp. 1351-1370 (2004).

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Scientific paper

We analyse the physical implications of the energy and matching conditions that take part in the construction of spherically symmetric models for stars and voids. We find an important condition on the radial pressures that can be of relevance, for instance, in the modellization of voids in the universe. In this way we show, among other results, that some models for the universe could not possess viable voids. The condition is also applied in order to construct charged radiating stellar models.

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