Thermodynamics of quantum spacetime histories

Lee Smolin
Phys. Rev. D 96, 104042 – Published 22 November 2017

Abstract

We show that the simplicity constraints, which define the dynamics of spin foam models, imply, and are implied by, the first law of thermodynamics, when the latter is applied to causal diamonds in the quantum spacetime. This result reveals an intimate connection between the holographic nature of gravity, as reflected by the Bekenstein entropy, and the fact that general relativity and other gravitational theories can be understood as constrained topological field theories. To state and derive this correspondence we describe causal diamonds in the causal structure of spin foam histories and generalize arguments given for the near horizon region of black holes by Frodden, Gosh and Perez [Phys. Rev. D 87, 121503 (2013); Phys. Rev. D 89, 084069 (2014); Phys. Rev. Lett. 107, 241301 (2011); Phys. Rev. Lett.108, 169901(E) (2012).] and Bianchi [arXiv:1204.5122.]. This allows us to apply a recent argument of Jacobson [Phys. Rev. Lett. 116, 201101 (2016).] to show that if a spin foam history has a semiclassical limit described in terms of a smooth metric geometry, that geometry satisfies the Einstein equations. These results suggest also a proposal for a quantum equivalence principle.

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  • Received 29 November 2015

DOI:https://doi.org/10.1103/PhysRevD.96.104042

© 2017 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Lee Smolin*

  • Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2J 2Y5, Canada and Department of Physics and Astronomy, University of Waterloo and Department of Philosophy, University of Toronto

  • *lsmolin@perimeterinstitute.ca

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Issue

Vol. 96, Iss. 10 — 15 November 2017

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