Slow-roll approximation in quantum cosmology

DOI10.1088/1361-6382/ABE143zbMath1481.83110arXiv2009.06282OpenAlexW3126339226MaRDI QIDQ5163369

Oliver Janssen

Publication date: 3 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.06282

zbMATH Keywords

inflationquantum cosmologyslow-roll approximationtunneling wave function

Mathematics Subject Classification ID

Associative rings of functions, subdirect products, sheaves of rings (16S60) Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Tunneling in quantum theory (81U26)

Related Items (1)

Review of the no-boundary wave function

Cites Work

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• Observational consequences of a landscape
• On the geometry of the string landscape and the swampland
• One-loop quantum cosmology: \(\zeta\)-function technique for the Hartle-Hawking wave function of the universe
• Two dimensional nearly De Sitter gravity
• Swampland constraints on no-boundary quantum cosmology
• New boundary conditions for \(\mathrm{AdS}_2\)
• Robustness of inflation to inhomogeneous initial conditions
• Sharp predictions from eternal inflation patches in D-brane inflation
• The effects of potential shape on inhomogeneous inflation
• Inflation and String Theory
• Wave function of the Universe
• Quantum Theory of Gravity. I. The Canonical Theory
• Axion landscape cosmology
• Brane inflation.
• The Swampland: Introduction and Review

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