Perturbative quantum gravity and Newton's law on a flat Robertson-Walker background.

DOI10.1016/S0550-3213(98)00528-8zbMath1041.83507arXivgr-qc/9801028MaRDI QIDQ1570712

N. Delaunay

Publication date: 11 July 2000

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9801028

Mathematics Subject Classification ID

Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45)

Related Items (9)

Quantum gravitational corrections for spinning particles ⋮ Some inconvenient truths ⋮ Finite field-dependent symmetries in perturbative quantum gravity ⋮ More on cosmological gravitational waves and their memories ⋮ Perturbative quantum gravity induced scalar coupling to electromagnetism ⋮ Quantum linear gravity in de Sitter universe on Gupta-Bleuler vacuum state ⋮ One-loop quantum gravitational backreaction on the local Hubble rate ⋮ The graviton one-loop effective action in cosmological space-times with constant deceleration ⋮ Back-reaction to dilaton-driven inflation

Cites Work

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• The quantum gravitational back-reaction on inflation
• Nonperturbative models for the quantum gravitational back-reaction on inflation
• The structure of perturbative quantum gravity on a de Sitter background
• Matter contributions to the expansion rate of the universe.
• Graviton fluctuations in de Sitter space
• Classical and quantum fields in de Sitter space
• Quantum Fields in Curved Space

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