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On the black hole interior in string theory

Abstract The potential behind the horizon of an eternal black hole in classical theories is described in terms of data that is available to an external observer — the reflection coefficient of a wave that scatters on the black hole. In GR and perturbative string theory (in α′), the potential is regu...

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Main Authors: Roy Ben-Israel, Amit Giveon, Nissan Itzhaki, Lior Liram
格式: Artigo
語言:Inglês
出版: SpringerOpen 2017-05-01
叢編:Journal of High Energy Physics
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在線閱讀:http://link.springer.com/article/10.1007/JHEP05(2017)094
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