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Thermodynamics of Spacetime: The Einstein Equation of State
1995
Physical Review Letters
The Einstein equation is derived from the proportionality of entropy and horizon area together with the fundamental relation δ Q=TdS connecting heat, entropy, and temperature. The key idea is to demand that this relation hold for all the local Rindler causal horizons through each spacetime point, with δ Q and T interpreted as the energy flux and Unruh temperature seen by an accelerated observer just inside the horizon. This requires that gravitational lensing by matter energy distorts the
doi:10.1103/physrevlett.75.1260
pmid:10060248
fatcat:n6setrd65rcgtofxawakvvlz6u