Gravitational collapse without a remnant
arXiv:0804.3892 · doi:10.1007/s10773-008-9681-6
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 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