Pressure of the Standard Model Near the Electroweak Phase Transition
arXiv:hep-ph/0512177 · doi:10.1088/1126-6708/2006/03/011
Abstract
We extend our previous determination of the thermodynamic pressure of the Standard Model so that the result can be applied down to temperatures corresponding to the electroweak crossover. This requires a further resummation which can be cleanly organised within the effective theory framework. The result allows for a precise determination of the expansion rate of the Universe for temperatures around the electroweak crossover.
16 pages, 6 figures. v2: published version
Cited by in corpus (20)
- Quark mass thresholds in QCD thermodynamics
- Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model
- The Standard Model cross-over on the lattice
- Theoretical uncertainties for cosmological first-order phase transitions
- Perturbative Thermal QCD: Formalism and Applications
- Standard Model thermodynamics across the electroweak crossover
- On the perturbative expansion at high temperature and implications for cosmological phase transitions
- Robust approach to thermal resummation: Standard Model meets a singlet
- Combining thermal resummation and gauge invariance for electroweak phase transition
- Computing the gauge-invariant bubble nucleation rate in finite temperature effective field theory
- Four-loop pressure of massless O(N) scalar field theory
- Three-dimensional effective theories for the two Higgs doublet model at high temperature
- The Electroweak Phase Transition in Ultra Minimal Technicolor
- Mesonic screening masses at high temperature and finite density
- Non-perturbative determination of the sphaleron rate for first-order phase transitions
- Soft contributions to the thermal Higgs width across an electroweak phase transition
- Entropy production at electroweak bubble walls from scalar field fluctuations
- Hard thermal contributions to phase transition observables at NNLO
- Nucleation at finite temperature: a gauge-invariant, perturbative framework
- Speed of sound in cosmological phase transitions and effect on gravitational waves