Schwarzschild Fuzzball and Explicitly Unitary Hawking Radiations
arXiv:1802.00675 · doi:10.1016/j.nuclphysb.2018.03.012
Abstract
We provide a fuzzball picture for Schwarzshild black holes, in which matters and energy consisting the hole are not positioned on the central point exclusively but oscillate around there in a serial of eigen-modes, each of which features a special level of binding degrees and are quantum mechanically possible to be measured outside the horizon. By listing these modes explicitly for holes as large as , we find that their number increases exponentially with the area. Basing on this picture, we present a simple but explicitly unitary derivation of hawking radiations.
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- Chaotic D1-D5 Black Hole Dynamics through Networks