Gravitational collapse without a remnant

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We investigate the gravitational collapse of a spherically symmetric, inhomogeneous star, which is described by a perfect fluid with heat flow and satisfies the equation of state $p=ρ/3$ or $p=Cρ^\ga$ at its center. Different from the ordinary process of gravitational collapsing, the energy of the whole star is emitted into space. And the remaining spacetime is a Minkowski one at the end of the process.
9 pages, 9 figures, to appear in Int. J. Theor. Phys

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/203481

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0804.3892
 http://arxiv.org/abs/0804.3892
 Int.J.Theor.Phys.47:2479-2491,2008
 doi:10.1007/s10773-008-9681-6

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arXiv