Holographic duality and mode stability of de Sitter space in semiclassical gravity

DOI10.1088/1475-7516/2020/11/010zbMath1486.83038arXiv2003.05501OpenAlexW3095324184MaRDI QIDQ5035272

Paul M. Chesler, Abraham Loeb

Publication date: 21 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2003.05501

zbMATH Keywords

gravityquantum gravity phenomenologydark energy theoryquantum field theory on curved space

Mathematics Subject Classification ID

Supergravity (83E50) Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Kaluza-Klein and other higher-dimensional theories (83E15) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Exact solutions to problems in general relativity and gravitational theory (83C15) Dark matter and dark energy (83C56)

Related Items

De Sitter quantum breaking, swampland conjectures and thermal strings ⋮ Back-reaction in massless de Sitter QFTs: holography, gravitational DBI action and f(R) gravity ⋮ Quantum (in)stability of maximally symmetric space-times ⋮ Holographic evolution with dynamical boundary gravity

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