Holographic evolution with dynamical boundary gravity

  • Holography has provided valuable insights into the time evolution of strongly coupled gauge theories in a fixed spacetime. However, this framework is insufficient if this spacetime is dynamical. We present a novel scheme to evolve a four-dimensional, strongly interacting gauge theory coupled to four-dimensional dynamical gravity in the semiclassical regime. We use holography to evolve the quantum gauge theory stress tensor. The four-dimensional metric evolves according to the four-dimensional Einstein equations coupled to the expectation value of the stress tensor. We focus on Friedmann-Lemaître-Robertson-Walker geometries and evolve far-from-equilibrium initial states that lead to asymptotically expanding, flat or collapsing Universes.

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Author:Christian EckerORCiD, Wilke van der ScheeORCiD, David MateosORCiD, Jorge Casalderrey-SolanaORCiDGND
URN:urn:nbn:de:hebis:30:3-837156
URL:https://arxiv.org/abs/2109.10355v1
DOI:https://doi.org/10.48550/arXiv.2109.10355
ArXiv Id:http://arxiv.org/abs/2109.10355v1
Parent Title (English):arXiv
Series (Serial Number):CERN Report (CERN-TH-2021-137)
Publisher:arXiv
Document Type:Preprint
Language:English
Date of Publication (online):2021/09/21
Date of first Publication:2021/09/21
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2024/04/30
Tag:QFT on curved background; cosmology; gauge/gravity duality; hydrodynamics
Issue:2109.10355 Version 1
Edition:Version 1
Page Number:5
HeBIS-PPN:518866726
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 4.0