The role of fluctuation-dissipation dynamics in setting initial conditions for inflation

DOI10.1088/1475-7516/2018/01/002OpenAlexW3100688863MaRDI QIDQ5021776

Rudnei O. Ramos, João G. Rosa, Mar Bastero-Gil, Arjun Berera, Ian G. Moss, Robert H. Brandenberger

Publication date: 14 January 2022

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

Full work available at URL: https://arxiv.org/abs/1612.04726

zbMATH Keywords

inflationphysics of the early universeparticle physics-cosmology connectioninitial conditions and eternal universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (4)

Scale-invariant scalar field dark matter through the Higgs portal ⋮ Setting initial conditions for inflation with reaction-diffusion equation ⋮ Theoretical cosmology ⋮ G-warm inflation

Uses Software

• GRChombo

Cites Work

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• The importance of being warm (during inflation)
• How likely are constituent quanta to initiate inflation?
• A new type of isotropic cosmological models without singularity
• GRChombo  : Numerical relativity with adaptive mesh refinement
• Finite-Temperature Field Theory
• WARM INFLATION MODEL BUILDING
• STRING GAS COSMOLOGY AND STRUCTURE FORMATION
• Nonperturbative dynamics of reheating after inflation: A review
• Robustness of inflation to inhomogeneous initial conditions
• Multi-phase induced inflation in theories with non-minimal coupling to gravity
• Inflationary universe: A possible solution to the horizon and flatness problems

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