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Relaxational effects in radiating stellar collapse

Megan Govender·Roy Maartens·Sunil Maharaj
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Abstract

Relaxational effects in stellar heat transport can in many cases be significant. Relativistic Fourier-Eckart theory is inherently quasi-stationary, and cannot incorporate these effects. The effects are naturally accounted for in causal relativistic thermodynamics, which provides an improved approximation to kinetic theory. Recent results, based on perturbations of a static star, show that relaxation effects can produce a significant increase in the central temperature and temperature gradient for a given luminosity. We use a simple stellar model that allows for non-perturbative deviations from staticity, and confirms qualitatively the predictions of the perturbative models.

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Megan Govender, Roy Maartens, Sunil Maharaj. 1998-10-01. Relaxational effects in radiating stellar collapse. https://doi.org/10.1046/j.1365-8711.1999.02963.x

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