Effective reheating in Gauss--Bonnet inflation with mu(phi,X) coupling
astro-ph.CO
Submitted: 2026-08-03
Updated: 2026-09-19
Comments: 25 pages, 7 figures, 9 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Reheating after Inflation
- Towards the Theory of Reheating After Inflation
- Reheating in Inflationary Cosmology: Theory and Applications
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- Reheating constraints to inflationary models
- Observing the Inflationary Reheating
- Equation-of-State Parameter for Reheating
- Reheating predictions in single field inflation
- The Equation of State and Duration to Radiation Domination After Inflation
- MeV-scale Reheating Temperature and Thermalization of Neutrino Background
- Bounds on very low reheating scenarios after Planck
- MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles
- Cosmological Constraints on Late-time Entropy Production
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Gauss-Bonnet dark energy
- Circular Polarization of Primordial Gravitational Waves in String-inspired Inflationary Cosmology
- Higher Curvature Corrections to Primordial Fluctuations in Slow-roll Inflation
- Power spectra from an inflaton coupled to the Gauss-Bonnet term
- Gauss-Bonnet Inflation
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