Gravitational collapse of a massive sphere of constant energy density

Details Gravitational collapse of a massive sphere of constant energy density Gravitational collapse of a massive sphere of constant energy density

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143..187d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 1, April 1988, p. 187-191. Research supported by the Department o

Statistics

Computation

Asymptotic Methods, Black Holes (Astronomy), Gravitational Collapse, Red Shift, Stellar Structure, Computational Astrophysics, Relativistic Theory, Stellar Mass

Scientific paper

Gravitational collapse of a massive sphere of constant density has been studied from the point of view of a Keplerian observer. The asymptotic nature of collapse is attributed to the development of negative gravitational pressure acting radially outwards within the structure. The region of negative pressure asymptotically covers the entire interior as u = mass/radius tends to half.

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