Massive fluid spheres in general relativity

Details Massive fluid spheres in general relativity Massive fluid spheres in general relativity

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..32.1358p&link_type=abstract

Physical Review D (Particles and Fields), Volume 32, Issue 6, 15 September 1985, pp.1358-1363

Computer Science

Sound

9

Exact Solutions, Neutron Stars

Scientific paper

We present a class of nonsingular analytic solutions of the general-relativistic field equations in isotropic form for a static spherically symmetric material distribution. Within a sphere the outward variation of pressure, density, pressure-density ratio, and the adiabatic sound speed is monotonic decreasing. The solution has been used to construct causal models for neutron stars with a maximum mass ~=4Mcirdot where we have assumed a surface density equivalent to the typical terrestrial nuclear density.

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