Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..375s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 2, April 1985, p. 375-381.
Astronomy and Astrophysics
Astrophysics
Equations Of State, Neutron Stars, Relativity, Stellar Gravitation, Stellar Mass, Field Strength, Red Shift, Schwarzschild Metric, Systems Stability
Scientific paper
The authors consider the possibility that gravitational energy may play a local as well as a global role in the behavior of matter in strong gravitational fields. A particular idealized equation, suggested as representing uniform energy density in general relativity, is examined, and its stability with respect to oscillatory and convective perturbations shown to be consistent with general relativistic hydrodynamics, subject to a new physical effect predicted for the behavior of fluids moving in strong fields. The authors calculate from this idealized equation the mass of a non-rotating neutron star.
Eccles M. J.
Sarracino R. S.
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