Rotating superdense configurations with allowance for pionization of matter

Details Rotating superdense configurations with allowance for pionization of matter Rotating superdense configurations with allowance for pionization of matter

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979afz....15..497h&link_type=abstract

(Astrofizika, vol. 15, July-Sept. 1979, p. 497-502.) Astrophysics, vol. 15, no. 3, Jan. 1980, p. 331-334. Translation.

Astronomy and Astrophysics

Astrophysics

Celestial Bodies, Density (Number/Volume), Equations Of State, Pions, Rotating Bodies, Celestial Mechanics, Equilibrium Equations, Ionization, Mass Distribution, Radii

Scientific paper

The parameters of rotating superdense celestial bodies are determined on
the basis of a new equation of state which accounts for the pionization
effect. Masses and radii of four static and rotating configurations
calculated with and without allowance for the pionization effect are
compared.

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