What is a chiral 2d CFT? And what does it have to do with extremal black holes?

被引:85
作者
Balasubramanian, Vijay [1 ]
de Boer, Jan [2 ]
Sheikh-Jabbari, M. M. [3 ,4 ]
Simon, Joan [5 ,6 ,7 ]
机构
[1] Univ Penn, David Rittenhouse Lab, Philadelphia, PA 19104 USA
[2] Inst Theoret Fys, NL-1018 XE Amsterdam, Netherlands
[3] Inst Res Fundamental Sci IPM, Sch Phys, Tehran, Iran
[4] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy
[5] Maxwell Inst Math Sci, Edinburgh EH9 3JZ, Midlothian, Scotland
[6] Sch Math, Edinburgh EH9 3JZ, Midlothian, Scotland
[7] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
基金
美国国家科学基金会; 英国工程与自然科学研究理事会;
关键词
Black Holes in String Theory; AdS-CFT Correspondence; FIELD-THEORIES; SYMMETRIES;
D O I
10.1007/JHEP02(2010)017
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 near horizon limit of the extremal BTZ black hole is a "self-dual orbifold" of AdS(3). This geometry has a null circle on its boundary, and thus the dual field theory is a Discrete Light Cone Quantized (DLCQ) two dimensional CFT. The same geometry can be compactified to two dimensions giving AdS(2) with a constant electric field. The kinematics of the DLCQ show that in a consistent quantum theory of gravity in these backgrounds there can be no dynamics in AdS(2), which is consistent with older ideas about instabilities in this space. We show how the necessary boundary conditions eliminating AdS(2) fluctuations can be implemented, leaving one copy of a Virasoro algebra as the asymptotic symmetry group. Our considerations clarify some aspects of the chiral CFTs appearing in proposed dual descriptions of the near-horizon degrees of freedom of extremal black holes.
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