A class of well behaved charged superdense star models of embedding class one

Details A class of well behaved charged superdense star models of embedding class one A class of well behaved charged superdense star models of embedding class one

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.336..419g&link_type=abstract

Astrophysics and Space Science, Volume 336, Issue 2, pp.419-426

Astronomy and Astrophysics

Astrophysics

1

Exact Solutions, Charged Fluids, Superdense Stars, General Relativity, Negative Redshift

Scientific paper

A class of well behaved charged superdense star models of embedding class one is obtained by taking perfect fluid to be interior matter. In the process we come across the models for white dwarf, quark and neutron stars. Maximum mass of the star of this class is found to be 6.716998 M Θ with its radius is 18.92112 Km. In the absence of charge the models reduce to Schwarzchild's interior model with constant density.

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