Abstract
Contradiction between Hawking's semi-classical arguments and the string theory on the evaporation of a black hole has been one of the most intriguing problems in fundamental physics. A final-state boundary condition inside the black hole was proposed by Horowitz and Maldacena to resolve this contradiction. We point out that the original Hawking effect can also be regarded as a separate boundary condition at the event horizon for this scenario. Here, we found that the change of the Hawking boundary condition may affect the information transfer from the initial collapsing matter to the outgoing Hawking radiation during the evaporation process and as a result the evaporation process itself, significantly.
Original language | English |
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Article number | 021 |
Journal | Journal of High Energy Physics |
Volume | 2007 |
Issue number | 3 |
DOIs | |
State | Published - 1 Mar 2007 |
Keywords
- Black holes
- Black holes in string theory