Quantum phenomenological gravitational dynamics: a general view from thermodynamics of spacetime

被引:12
|
作者
Alonso-Serrano, A. [1 ]
Liska, M. [2 ]
机构
[1] Max Planck Inst Gravitat Phys, Albert Einstein Inst, Muhlenberg 1, D-14476 Potsdam, Germany
[2] Charles Univ Prague, Fac Math & Phys, Inst Theoret Phys, Holesovickach 2, Prague 18000 8, Czech Republic
关键词
Models of Quantum Gravity; Spacetime Singularities; Black Holes; Classical Theories of Gravity; BLACK-HOLE ENTROPY; LOGARITHMIC CORRECTIONS; COSMOLOGICAL CONSTANT;
D O I
10.1007/JHEP12(2020)196
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
In this work we derive general quantum phenomenological equations of gravitational dynamics and analyse its features. The derivation uses the formalism developed in thermodynamics of spacetime and introduces low energy quantum gravity modifications to it. Quantum gravity effects are considered via modification of Bekenstein entropy by an extra logarithmic term in the area. This modification is predicted by several approaches to quantum gravity, including loop quantum gravity, string theory, AdS/CFT correspondence and generalised uncertainty principle phenomenology, giving our result a general character. The derived equations generalise classical equations of motion of unimodular gravity, instead of the ones of general relativity, and they contain at most second derivatives of the metric. We provide two independent derivations of the equations based on thermodynamics of local causal diamonds. First one uses Jacobson's maximal vacuum entanglement hypothesis, the second one Clausius entropy flux. Furthermore, we consider questions of diffeomorphism and local Lorentz invariance of the resulting dynamics and discuss its application to a simple cosmological model, finding a resolution of the classical singularity.
引用
收藏
页数:31
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