The effect of backreaction on inflationary Starobinsky cosmology

DOI10.1142/S0219887817501341zbMath1376.83035OpenAlexW2614003672MaRDI QIDQ5370547

M. Sahraee, Mohammad R. Setare

Publication date: 20 October 2017

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887817501341

zbMATH Keywords

energy-momentum tensorWKB approximationquantum fieldvacuum expectation valuescale factorbackreactiontrace anomalyspatially flat \(D\)-dimensional Friedmann-Robertson-Walker universeStarobinsky cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Kaluza-Klein and other higher-dimensional theories (83E15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

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• Quantum Field Theory in Curved Spacetime
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• Inflationary universe: A possible solution to the horizon and flatness problems
• Quantum Fields in Curved Space

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