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arXiv · 1111.4921

Radiating Shear-Free Gravitational Collapse with Charge

G. Pinheiro·R. Chan
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Abstract

We present a new shear free model for the gravitational collapse of a spherically symmetric charged body. We propose a dissipative contraction with radiation emitted outwards. The Einstein field equations, using the junction conditions and an ansatz, are integrated numerically. A check of the energy conditions is also performed. We obtain that the charge delays the black hole formation and it can even halt the collapse.

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G. Pinheiro, R. Chan. 2011-11-21. Radiating Shear-Free Gravitational Collapse with Charge. https://doi.org/10.1007/s10714-012-1468-7

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