Thermodynamics of Spacetime: The Einstein Equation of State
Ted Jacobson

TL;DR
This paper derives Einstein's field equations from thermodynamic principles, interpreting them as an equation of state related to horizon entropy and heat flux, and suggests a thermodynamic perspective on gravity.
Contribution
It presents a novel derivation of Einstein's equations from entropy and heat relations at local horizons, framing gravity as an emergent thermodynamic phenomenon.
Findings
Einstein equation derived from thermodynamic relations at horizons
Gravity viewed as an equation of state, not fundamental quantized field
Supports emergent gravity perspective
Abstract
The Einstein equation is derived from the proportionality of entropy and horizon area together with the fundamental relation 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 and 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 causal structure of spacetime in just such a way that the Einstein equation holds. Viewed in this way, the Einstein equation is an equation of state. This perspective suggests that it may be no more appropriate to canonically quantize the Einstein equation than it would be to quantize the wave equation for sound in air.
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