The kinematics of cosmic reheating

DOI10.1016/j.nuclphysb.2013.07.009zbMath1282.83067arXiv1305.0267OpenAlexW2078630190MaRDI QIDQ2438244

Marco Drewes, Jin U Kang

Publication date: 10 March 2014

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

Full work available at URL: https://arxiv.org/abs/1305.0267

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Yang-Mills and other gauge theories in quantum field theory (81T13) Transport processes in time-dependent statistical mechanics (82C70) Statistical mechanics of plasmas (82D10) Dispersion theory, dispersion relations arising in quantum theory (81U30) Thermal quantum field theory (81T28)

Related Items (17)

Reheating constraints to modulus mass for single field inflationary models ⋮ Effective action for cosmological scalar fields at finite temperature ⋮ Towards a precision calculation of the effective number of neutrinos N_eff in the Standard Model: the QED equation of state ⋮ General Markovian equation for scalar fields in a slowly evolving background ⋮ Measuring inflaton couplings via primordial gravitational waves ⋮ Dissipation of oscillating scalar backgrounds in an FLRW universe ⋮ Backreaction effects on nonequilibrium spectral function ⋮ Symmetric and asymmetric reheating ⋮ CMB constraints on the inflaton couplings and reheating temperature in \(\alpha\)-attractor inflation ⋮ Novel collective excitations in a hot scalar field theory ⋮ Fate of \(Z_{2}\) symmetric scalar field ⋮ Effective field theory out of equilibrium: Brownian quantum fields ⋮ Nonperturbative dynamics of reheating after inflation: A review ⋮ Oscillating scalar dissipating in a medium ⋮ Boltzmann equations for preheating ⋮ Reconciling low multipole anomalies and reheating in single field inflationary models ⋮ Thermal gravitational-wave background in the general pre-inflationary scenario

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