Isothermal neutron star core

Details Isothermal neutron star core Isothermal neutron star core

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jpha...12..859d&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 12, June 1979, p. 859-862.

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11

Equilibrium Equations, Isothermal Processes, Neutron Stars, Stellar Mass, Cores, Density Distribution, Equations Of State, Hydrostatics

Scientific paper

The equations of hydrostatic equilibrium are solved for the equation of state P = K x rho, for finite central densities and K not less than 1/3. It is found that, surprisingly, the maximum mass of the neutron star core occurs at the K = 0.80 and not at K = 1.00. The masses of these cores lie between 2.1 and 2.5 solar masses and the maximum mass value occurs at almost the same central density, i.e., 3 x 10 to the 15th g/cu cm.

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