Radiating gravitational collapse before relaxation

Physics

Scientific paper

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Scientific paper

The study of the gravitational collapse of a radiating sphere is carried out for times shorter than the effective time of relaxation into diffusion. Using a relativistic version of the Cattaneo equation for the heat flux, we show with an explicit example that processes occurring before relaxation give rise to luminosity profiles which are quite different from the profiles corresponding to vanishing relaxation time, leading thereby to very different patterns of evolution.

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