Energy distribution and equation of state of the early universe: matching the end of inflation and the onset of radiation domination
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Publication:820355
DOI10.1016/j.physletb.2020.135888zbMath1475.83127arXiv2005.07563OpenAlexW3025737699MaRDI QIDQ820355
Daniel G. Figueroa, Kenneth Marschall, Francisco Torrenti, Stefan Antusch
Publication date: 27 September 2021
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2005.07563
Related Items (6)
Characterizing the post-inflationary reheating history. Part II. Multiple interacting daughter fields ⋮ Model independent results for the inflationary epoch and the breaking of the degeneracy of models of inflation ⋮ Dark matter production and reheating via direct inflaton couplings: collective effects ⋮ Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation ⋮ Aspects of wave turbulence in preheating III: The case of the two-field models ⋮ WIMPs during reheating
Uses Software
Cites Work
- \texttt{LATTICEEASY}: A program for lattice simulations of scalar fields in an expanding universe
- \texttt{CLUSTEREASY}: A program for lattice simulations of scalar fields in an expanding universe on parallel computing clusters
- A new type of isotropic cosmological models without singularity
- Nonperturbative dynamics of reheating after inflation: A review
- (P)reheating after minimal plateau inflation and constraints from CMB
- Ability of LIGO and LISA to probe the equation of state of the early Universe
- Metric preheating and radiative decay in single-field inflation
- Inflationary universe: A possible solution to the horizon and flatness problems
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