Elliptic Genera and 3d Gravity

被引:24
|
作者
Benjamin, Nathan [1 ,2 ]
Cheng, Miranda C. N. [3 ,4 ]
Kachru, Shamit [1 ,2 ]
Moore, Gregory W. [5 ,6 ]
Paquette, Natalie M. [1 ,2 ]
机构
[1] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[2] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[3] Univ Amsterdam, Inst Phys, Amsterdam, Netherlands
[4] Univ Amsterdam, Korteweg de Vries Inst Math, Amsterdam, Netherlands
[5] Rutgers State Univ, NHETC, Piscataway, NJ 08855 USA
[6] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08855 USA
来源
ANNALES HENRI POINCARE | 2016年 / 17卷 / 10期
基金
美国国家科学基金会;
关键词
BLACK-HOLES;
D O I
10.1007/s00023-016-0469-6
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We describe general constraints on the elliptic genus of a 2d supersymmetric conformal field theory which has a gravity dual with large radius in Planck units. We give examples of theories which do and do not satisfy the bounds we derive, by describing the elliptic genera of symmetric product orbifolds of K3, product manifolds, certain simple families of Calabi-Yau hypersurfaces, and symmetric products of the "Monster CFT". We discuss the distinction between theories with supergravity duals and those whose duals have strings at the scale set by the AdS curvature. Under natural assumptions, we attempt to quantify the fraction of (2,2) supersymmetric conformal theories which admit a weakly curved gravity description, at large central charge.
引用
收藏
页码:2623 / 2662
页数:40
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