Microscopic properties of black holes in string theory

被引：0

作者：

Cvetic, M ^{[1
]}

机构：

[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

来源：

BEYOND THE DESERT 1999: ACCELERATOR, NON-ACCELERATOR AND SPACE APPROACHES INTO THE NEXT MILLENNIUM | 1999年

关键词：

D O I：

暂无

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：

We review the status of microscopic counting of black hole degrees of freedom. We present complementary approaches which utilize the near-horizon geometry and precisely reproduce the Bekenstein Hawking entropy for near-extreme rotating black holes in D=4 and D=5. One relies on the correspondence between the near-horizon geometry and the conformal field theory on its boundary (AdS/CFT correspondence) and another one employs the conformal sigma-model in the Neveu-Schwarz-Neveu-Schwarz sector and accounts for the black hole microstates by counting the small scale oscillations of the dyonic string there.

引用

页码：359 / 372

页数：14