Jackiw-Teitelboim gravity in the second order formalism

被引:18
|
作者
Moitra, Upamanyu [1 ]
Sake, Sunil Kumar [1 ]
Trivedi, Sandip P. [1 ]
机构
[1] Tata Inst Fundamental Res, Dept Theoret Phys, Mumbai 400005, Maharashtra, India
关键词
2D Gravity; Black Holes; Models of Quantum Gravity; QUANTUM; DETERMINANTS;
D O I
10.1007/JHEP10(2021)204
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 formulate the path integral for Jackiw-Teitelboim gravity in the second order formalism working directly with the metric and the dilaton. We consider the theory both in Anti-de Sitter(AdS) and de Sitter space(dS) and analyze the path integral for the disk topology and the "double trumpet" topology with two boundaries. We also consider its behavior in the presence of conformal matter. In the dS case the path integral evaluates the wavefunction of the universe which arises in the no-boundary proposal. In the asymptotic AdS or dS limit without matter we get agreement with the first order formalism. More generally, away from this limit, the path integral is more complicated due to the presence of modes from the gravity-dilaton sector and also matter sector with short wavelengths along the boundary that are smaller than the AdS or dS scales. In the double trumpet case, for both AdS and dS, we find that bosonic matter gives rise to a diverging contribution in the moduli space integral rendering the path integral ill-defined. The divergence occurs when the size of the wormhole neck vanishes and is related to the Casimir effect. For fermions this divergence can be avoided by imposing suitable boundary conditions. In this case, in dS space the resulting path integral gives a finite contribution for two disconnected universes to be produced by quantum tunneling.
引用
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页数:103
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