Emergence of Spacetime: From Entanglement to Einstein
Andrew Svesko

TL;DR
This paper explores how thermodynamics and entanglement underpin the emergence of spacetime and gravity, deriving Einstein's equations from thermodynamic principles and providing microscopic insights via holography.
Contribution
It establishes a novel connection between thermodynamics, entanglement, and gravity, deriving Einstein's equations from local thermodynamic laws and extending the entanglement equilibrium framework.
Findings
Derives the null energy condition from thermodynamics.
Provides a microscopic explanation of thermodynamic volume in AdS/CFT.
Extends the first law of entanglement to lower-dimensional gravity models.
Abstract
Here I develop the connection between thermodynamics, entanglement, and gravity. I begin by showing that the classical null energy condition (NEC) can arise as a consequence of the second law of thermodynamics applied to local holographic screens. This is accomplished by essentially reversing the steps of Hawking's area theorem, leading to the Ricci convergence condition as an input, from which an application of Einstein's equations yields the NEC -- even in the presence of 1-loop quantum corrections to the Bekenstein-Hawking entropy formula. Then, by attributing thermodynamics to the stretched horizon of future lightcones -- a timelike hypersurface generated by a collection of radially accelerating observers with constant and uniform proper acceleration -- I derive Einstein's equations from the Clausius relation , where is the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
