1111.4921 (G. Pinheiro et al.)
G. Pinheiro, R. Chan
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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http://arxiv.org/abs/1111.4921
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