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General proof of the entropy principle for self-gravitating fluid in static spacetimes. 高思杰 (Gao Sijie) 北京师范大学 (Beijing Normal University). Outline. Introduction Entropy principle in spherical case --radiation Entropy principle in spherical case –perfect fluid
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General proof of the entropy principle for self-gravitating fluid in static spacetimes 高思杰 (Gao Sijie) 北京师范大学 (Beijing Normal University) 2014 Institute of Physics, Academia Sinica
Outline • Introduction • Entropy principle in spherical case --radiation • Entropy principle in spherical case –perfect fluid • Entropy principle in static spacetime • Related works • Conclusions. 2014 Institute of Physics, Academia Sinica
1. Introduction Mathematical analogy beween thermodynamics and black holes: 2014 Institute of Physics, Academia Sinica
What is the relationship between ordinary thermodynamics and gravity? We shall study thermodynamics of self-gravitating fluid in curved spacetime. 2014 Institute of Physics, Academia Sinica
Consider a self-gravitating perfect fluid with spherical symmetry in thermal equilibrium: S: total entropy of fluid M: total mass of fluid N: total particle number fluid There are two ways to determine the distribution of the fluid: 1. General relativity: Einstein’s equation gives Tolman-Oppenheimer-Volkoff (TOV ) equation: 2. Thermodynamics: at thermal equilibrium. Are they consistent?
2. Entropy principle in spherical case---radiation Sorkin, Wald, Zhang, Gen.Rel.Grav. 13, 1127 (1981) In 1981, Sorkin, Wald, and Zhang (SWZ) derived the TOV equation of a self-gravitating radiation from the maximum entropy principle. Proof: The stress-energy tensor is given by The radiation satisfies: 2014 Institute of Physics, Academia Sinica
Assume the metric of the spherically symmetric radiation takes the form The constraint Einstein equation yields 2014 Institute of Physics, Academia Sinica
Since , the extrema of is equivalent to the Euler-Lagrange equation: 2014 Institute of Physics, Academia Sinica
Using to replace , , we arrive at the TOV equation 2014 Institute of Physics, Academia Sinica
3. Entropy principle in spherical case---general perfect fluid (Sijie Gao, arXiv:1109.2804,Phys. Rev. D 84, 104023 ) • To generalize SWZ’s treatment to a general fluid, we first need to find an expression for the entropy density . • The first law of the ordinary thermodynamics: Rewrite in terms of densities: Expand: The first law in a unit volume: 2014 Institute of Physics, Academia Sinica
Thus, we have the Gibbs-Duhem relation 2014 Institute of Physics, Academia Sinica
Note that Thus,
4.Proof of the entropy principle for perfect fluid in static spacetimesarXiv: 1311.6899 • In this work, we present two theorems relating the total entropy of fluid to Einstein’s equation in any static spacetimes. • A static spacetime admits a timelike Killing vector field which is hypersurface orthogonal. 2014 Institute of Physics, Academia Sinica
Proof of Theorem 1 2014 Institute of Physics, Academia Sinica
The total entropy Its variation: Total number of particle: The constraint 2014 Institute of Physics, Academia Sinica
Then 2014 Institute of Physics, Academia Sinica
(Constraint Einstein equation) 2014 Institute of Physics, Academia Sinica
Integration by parts: Integration by parts again and dropping the boundary terms: 2014 Institute of Physics, Academia Sinica
5. Related works • Proof for stationary case----in process • Stability analysis (1) Z.Roupas [Class. Quantum Grav. 30, 115018 (2013)] calculated the second variation of entropy, showing that the stability of thermal equilibrium is equivalent to stability of Einstein’s equations. (2) Wald et. al. [Class. Quantum Grav. 31 (2014) 035023 ] proved the equivalence of dynamic equibrium and thermodynamic equibrium for stationary asymtotically flat spacetimes with axisymmetry. • Beyond general relativity: Li-Ming Cao, Jianfei Xu, Zhe Zeng [Phys. Rev. D 87, 064005 (2013)] proved the maximum entropy principle in the framework of Lovelock gravity. 2014 Institute of Physics, Academia Sinica
6. Conclusions • We have rigorously proven the equivalence of the extrema of entropy and Einstein's equation under a few natural and necessary conditions. The significant improvement from previous works is that no spherical symmetry or any other symmetry is needed on the spacelike hypersurface. Our work suggests a clear connection between Einstein's equation and thermodynamics of perfect fluid in static spacetimes. 2014 Institute of Physics, Academia Sinica
Thank you! 2014 Institute of Physics, Academia Sinica