From entanglement to thermodynamics and to gravity

被引:16
|
作者
Svesko, Andrew [1 ,2 ]
机构
[1] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA
[2] Arizona State Univ, Beyond Ctr Fundamental Concepts Sci, Tempe, AZ 85287 USA
关键词
BLACK-HOLE ENTROPY; NOETHER CHARGE; SPACETIME;
D O I
10.1103/PhysRevD.99.086006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Here we develop the connection between thermodynamics, entanglement, and gravity. By attributing thermodynamics to time slices of a causal diamond, we show that the Clausius relation T Delta S-rev = Q, where Delta S-rev is the reversible entropy change, gives rise to the nonlinear gravitational equations of motion for a wide class of diffeomorphism invariant theories. We then compare the Clausius relation to the first law of causal diamond mechanics (FLCD), a geometric identity and necessary ingredient in deriving Jacobson's entanglement equilibrium proposal-the entanglement entropy of a spherical region with a fixed volume is maximal in vacuum. Specifically we show that the condition of fixed volume can be understood as subtracting the irreversible contribution to the thermodynamic entropy. This provides a "reversible thermodynamic process" interpretation of the FLCD and that the condition of entanglement equilibrium may be regarded as equilibrium thermodynamics for which the Clausius relation holds. Finally, we extend the entanglement equilibrium proposal to the timelike stretched horizons of future light cones, providing an entanglement interpretation of stretched light cone thermodynamics.
引用
收藏
页数:24
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