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Gravitational Collapse without a Remnant
Authors:Zhe Chang  Cheng-Bo Guan  Chao-Guang Huang  Xin Li
Institution:(1) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;(2) Department of Space Science and Applied Physics, Shandong University, Weihai, 264209, China
Abstract: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=C ρ γ 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.
Keywords:Gravitational collapse  Inhomogeneous star  Energy mechanism for gamma-ray bursts
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