Contribution to the theory of superdense celestial bodies

Details Contribution to the theory of superdense celestial bodies Contribution to the theory of superdense celestial bodies

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56.1030g&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, Sept.-Oct. 1979, p. 1030-1036. In Russian.

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Celestial Bodies, Dense Plasmas, Supermassive Stars, Equations Of State, Mass Distribution, Mesons, Pressure Distribution

Scientific paper

Saakian and Grigorian (1977) have derived a new equation of state, in the form of a relationship between mass density and pressure, in the relativistic theory of superdense stars. In the present paper, the parameters of stars consisting of a degenerate neutron gas, calculated on the basis of the new equation of state with allowance for the pionization effect and the incompressibility of nuclear matter are examined.

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