Holographic framework for eternal inflation

被引:96
作者
Freivogel, Ben [1 ]
Sekino, Yasuhiro
Susskind, Leonard
Yeh, Chen-Pin
机构
[1] Univ Calif Berkeley, Dept Phys, Ctr Theoret Phys, Berkeley, CA 94720 USA
[2] Lawrence Berkeley Natl Lab, Berkeley, CA USA
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[4] Okayama Inst Quantum Phys, Okayama 7000015, Japan
来源
PHYSICAL REVIEW D | 2006年 / 74卷 / 08期
关键词
D O I
10.1103/PhysRevD.74.086003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we provide some circumstantial evidence for a holographic duality between bubble nucleation in an eternally inflating universe and a Euclidean conformal field theory (CFT). The holographic correspondence (which is different than Strominger's de Sitter (dS)/CFT duality) relates the decay of (3+1)-dimensional de Sitter space to a two-dimensional CFT. It is not associated with pure de Sitter space, but rather with Coleman-De Luccia bubble nucleation. Alternatively, it can be thought of as a holographic description of the open, infinite, Friedmann-Robertson-Walker (FRW) cosmology that results from such a bubble. The conjectured holographic representation is of a new type that combines holography with the Wheeler-DeWitt formalism to produce a Wheeler-DeWitt theory that lives on the spatial boundary of a k=-1 FRW cosmology. We also argue for a more ambitious interpretation of the Wheeler-DeWitt CFT as a holographic dual of the entire Landscape.
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页数:24
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