Statistics – Computation
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.200..271p&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 200, no. 2, p. 271-278.
Statistics
Computation
2
Computational Astrophysics, Neutron Stars, Stellar Interiors, Stellar Models, Condensed Matter Physics, Density Distribution, Maxwell Equation
Scientific paper
Consideration is given to a Reissner-Nordstrom interior solution of the Einstein-Maxwell equations for a charged superdense star. The ratio of central density to the radius for different values of lambda and the respective relevant quantities are calculated. It is found that the minimum radius density occurs when lambda attains the maximum possible value of 0.68, which is in excellent agreement with the estimation by Parui and Sarma (1991).
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