Effective action for cosmological scalar fields at finite temperature
From MaRDI portal
Publication:2635706
DOI10.1007/JHEP08(2015)059zbMath1388.83901arXiv1504.04444OpenAlexW3103385968MaRDI QIDQ2635706
Yeuk-Kwan E. Cheung, Jong Chol Kim, Jin U Kang, Marco Drewes
Publication date: 31 May 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1504.04444
cosmology of theories beyond the SMquantum dissipative systemsthermal field theoryeffective field theories
Related Items (5)
Energy spectrum of thermalizing high energy decay products in the early universe ⋮ General Markovian equation for scalar fields in a slowly evolving background ⋮ CMB constraints on the inflaton couplings and reheating temperature in \(\alpha\)-attractor inflation ⋮ Oscillating scalar dissipating in a medium ⋮ Superradiance in stars: non-equilibrium approach to damping of fields in stellar media
Cites Work
- Unnamed Item
- The Boltzmann equation from quantum field theory
- Bouncing universe and non-BPS branes
- Finite width in out-of-equilibrium propagators and kinetic theory
- Baryon washout, electroweak phase transition, and perturbation theory
- Novel collective excitations in a hot scalar field theory
- Strong electroweak phase transitions in the Standard Model with a singlet
- Fate of \(Z_{2}\) symmetric scalar field
- Quantifying the reheating temperature of the universe
- Calabi-Yau metrics and string compactification
- Nonequilibrium dynamics of scalar fields in a thermal bath
- Stochastic interpretation of Kadanoff-Baym equations and their relation to in processes
- A critical review of classical bouncing cosmologies
- A new type of isotropic cosmological models without singularity
- The kinematics of cosmic reheating
- Brownian Motion of a Quantum Oscillator
- Effective field theory out of equilibrium: Brownian quantum fields
- DYNAMICS OF DARK ENERGY
- Two-loop scalar self-mass during inflation
- Nonperturbative dynamics of reheating after inflation: A review
- Expectation Value Formalism in Quantum Field Theory. I
- Inflationary universe: A possible solution to the horizon and flatness problems
- \(k\)-inflation
- Infrared dynamics in de Sitter space from Schwinger-Dyson equations
This page was built for publication: Effective action for cosmological scalar fields at finite temperature