The maximum limit of the density variation parameter lambda for a stable neutron star

Details The maximum limit of the density variation parameter lambda for a stable neutron star The maximum limit of the density variation parameter lambda for a stable neutron star

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.186...81p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 186, no. 1, Dec. 1991, p. 81-87.

Statistics

Computation

3

Computational Astrophysics, Density Distribution, Neutron Stars, Stellar Models, Stellar Structure, Einstein Equations, Stellar Mass

Scientific paper

A static spherically-symmetric model, based on an exact solution of Einstein's equation, gives the permissible matter density about 2 x 10 exp 14 g/cu cm. If the change in the ratio of central density to the radius r = a minimum is used, the upper limit of the density variation parameter (lambda) and minimum mass limit of a superdense star like a neutron star is estimated. This limit gives an idea of the domain where the neutron abundance with negligible number of electrons and protons and equilibrium in neutrons begins.

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