Black Hole Evaporation along Macroscopic Strings
arXiv:hep-th/9312127 · doi:10.1103/PhysRevD.50.2680
Abstract
We develop the quantization of a macroscopic string which extends radially from a Schwarzschild black hole. The Hawking process excites a thermal bath of string modes that causes the black hole to lose mass. The resulting typical string configuration is a random walk in the angular coordinates. We show that the energy flux in string excitations is approximately that of spacetime field modes.
26pp, EFI 93-73. (Original claim that string Hawking flux exceeds spacetime flux is WRONG. It is the same; revised version provides correct argument and additional comments.)
References in corpus (5)
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