Macroscopic and microscopic gravitational fields in the study of gravitational collapse

Details Macroscopic and microscopic gravitational fields in the study of gravitational collapse Macroscopic and microscopic gravitational fields in the study of gravitational collapse

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ncimb..52..177b&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 52B, Aug. 11, 1979, p. 177-186. In French.

Physics

Field Theory (Physics), Gravitational Collapse, Gravitational Fields, Stellar Gravitation, Dynamic Response, Einstein Equations, Spheres, Stellar Structure

Scientific paper

The collapse of a spherical star without rotation is analyzed using
field equations derived by a method of averages. The two main features
of the solution are that the surface of the star does not exceed the
gravitational radius and that the density is always finite. The results
are interpreted in the framework of Hoyle's field theory.

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