Structures with extreme relativistic cores

Details Structures with extreme relativistic cores Structures with extreme relativistic cores

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jpha...13.3761d&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 13, Dec. 1980, p. 3761-3768. Research supported by the University Grants

Physics

3

Neutron Stars, Relativistic Theory, Stellar Structure, Polytropic Processes, Pulsars, Red Shift, Stellar Envelopes

Scientific paper

Stellar structures with extreme relativistic cores are considered (dP/d rho = 1 and 1/3). Central redshifts are calculated for the case of polytropic envelopes. It is found that the structures are pulsationally stable for Zc not greater than 1.43 when the polytropic index n = 1; for n less than 1, it is possible to obtain a central redshift of 4.75 for pulsationally stable structures. The mass of neutron stars is calculated, assuming the surface density to be 2 x 10 to the 14th g/cu cm; a maximum mass of 4.7 solar masses is obtained.

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