On radiating stellar collapse with shear

Details On radiating stellar collapse with shear On radiating stellar collapse with shear

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.299..809g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 299, Issue 3, pp. 809-810.

Astronomy and Astrophysics

Astronomy

3

Gravitation, Relativity, Stars: Interiors

Scientific paper

Relativistic models of radiating stellar collapse with shear require careful checking of all the equations and quantities involved. We illustrate this by showing that, in a recently proposed model, the metric ansatz is in fact too restrictive to allow any radial evolution to occur, and only tangential evolution is possible. Furthermore, the assumption of pressure isotropy is shown to reduce the model to the static case without radiation or shear.

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