Energy conditions allow eternal inflation

DOI10.1088/1475-7516/2021/03/097zbMath1485.83153arXiv2008.01878OpenAlexW3139718875MaRDI QIDQ5026066

Eleni-Alexandra Kontou, Ken D. Olum

Publication date: 7 February 2022

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

Full work available at URL: https://arxiv.org/abs/2008.01878

zbMATH Keywords

gravityinflationquantum cosmologyquantum field theory on curved space

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Geometrodynamics and the holographic principle (83E05) Quantization of the gravitational field (83C45)

Related Items (2)

How Different Connections in Flat FLRW Geometry Impact Energy Conditions in f(Q)$f(Q)$ Theory? ⋮ Cosmic bounce and phantom-like equation of state from tunnelling

Cites Work

• Unnamed Item
• EFT beyond the horizon: stochastic inflation and how primordial quantum fluctuations go classical
• Stress tensor fluctuations and passive quantum gravity
• DYNAMICAL BACKREACTION IN ROBERTSON–WALKER SPACETIME
• Semiclassicality and decoherence of cosmological perturbations
• QUANTUM-TO-CLASSICAL TRANSITION FOR FLUCTUATIONS IN THE EARLY UNIVERSE
• Semiclassical p-branes in hyperbolic space
• Uniqueness of de Sitter space
• Inflationary universe: A possible solution to the horizon and flatness problems

This page was built for publication: Energy conditions allow eternal inflation