Contraction of Radiating Shell in Classical and Post-Newtonian Approximation

Details Contraction of Radiating Shell in Classical and Post-Newtonian Approximation Contraction of Radiating Shell in Classical and Post-Newtonian Approximation

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.268..469s&link_type=abstract

Astrophysics and Space Science, v. 268, Issue 4, p. 469-474 (1999).

Astronomy and Astrophysics

Astrophysics

Scientific paper

A semi-numeric method was used to study the evolution of a
general-relativistic radiating shell in its Post-Newtonian and Newtonian
approximations. The solutions, where the main parameters are given
reasonable values, show that a relativistic effect can be found in
X-ray-burster-like objects.

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