Models of incompressible fluid configurations with allowance for the part played by the gravitational vacuum

Details Models of incompressible fluid configurations with allowance for the part played by the gravitational vacuum Models of incompressible fluid configurations with allowance for the part played by the gravitational vacuum

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....21..367g&link_type=abstract

(Astrofizika, vol. 21, Sept.-Oct. 1984, p. 367-377) Astrophysics (ISSN 0571-7132), vol. 20, no. 5, March 1985, p. 551-557. Trans

Astronomy and Astrophysics

Astrophysics

Einstein Equations, Gravitational Effects, Incompressible Fluids, Space-Time Functions, Stellar Models, Vacuum, Baryons, Minkowski Space, Schwarzschild Metric, Stellar Evolution, Stellar Magnitude, Vacuum Effects

Scientific paper

Models of superdense incompressible fluid stellar configurations are calculated under the assumption of Grigorian ad Saakian (1984) that a special gravitational vacuum exists. In the case of superdense celestial bodies, vacuum effects are important. The most important result is the conclusion that equilibrium superdense celestial bodies with masses much greater than the sun's can exist.

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