On the black hole interior in string theory

被引：10

作者：

Ben-Israel, Roy ^{[1
]}

Giveon, Amit ^{[2
]}

Itzhaki, Nissan ^{[1
]}

Liram, Lior ^{[1
]}

机构：

[1] Tel Aviv Univ, Phys Dept, IL-69978 Ramat Aviv, Israel

[2] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2017年 / 05期

基金：

以色列科学基金会;

关键词：

Black Holes in String Theory; Black Holes; Spacetime Singularities; SCATTERING;

D O I：

10.1007/JHEP05(2017)094

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

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 alpha '), the potential is regular at the horizon and it blows up at the singularity. The exact reflection coefficient, that is known for the SL(2,R)(k)/U(1) black hole and includes non-perturbative alpha ' effects, seems however to imply that there is a highly non-trivial structure just behind the horizon.

引用

页数：16

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