Quantum compositeness of gravity: black holes, AdS and inflation

被引:142
|
作者
Dvali, Gia [1 ,2 ,3 ]
Gomez, Cesar [1 ,4 ]
机构
[1] Univ Munich, Arnold Sommerfeld Ctr Theoret Phys, Dept Phys, D-80333 Munich, Germany
[2] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany
[3] NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA
[4] Univ Autonoma Madrid, CSIC, C XVI, Inst Fis Teor, E-28049 Madrid, Spain
基金
美国国家科学基金会;
关键词
inflation; gravity; cosmological perturbation theory; dark energy theory; THERMODYNAMICS; LIMIT;
D O I
10.1088/1475-7516/2014/01/023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Gravitational backgrounds, such as black holes, AdS, de Sitter and inflationary universes, should be viewed as composite of N soft constituent gravitons. It then follows that such systems are close to quantum criticality of graviton Bose-gas to Bose-liquid transition. Generic properties of the ordinary metric description, including geodesic motion or particle-creation in the background metric, emerge as the large-N limit of quantum scattering of constituent longitudinal gravitons. We show that this picture correctly accounts for physics of large and small black holes in AdS, as well as reproduces well-known inflationary predictions for cosmological parameters. However, it anticipates new effects not captured by the standard semi-classical treatment. In particular, we predict observable corrections that are sensitive to the inflationary history way beyond last 60 e-foldings. We derive an absolute upper bound on the number of e-foldings, beyond which neither de Sitter nor inflationary Universe can be approximated by a semi-classical metric. However, they could in principle persist in a new type of quantum eternity state. We discuss implications of this phenomenon for the cosmological constant problem.
引用
收藏
页数:47
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