Pressure of the Standard Model at High Temperatures
arXiv:hep-ph/0510375 · doi:10.1088/1126-6708/2006/01/060
Abstract
We compute the pressure of the standard model at high temperatures in the symmetric phase to three loops, or to O(g^5) in all coupling constants. We find that the terms of the perturbative expansion in the SU(2) + Higgs sector decrease monotonically with increasing order, but the large values of the strong coupling constant g_s and the Yukawa coupling of the top quark g_Y make the expansion in the full theory converge more slowly. The final result is observed to be about 10% smaller than the ideal gas pressure commonly used in cosmological calculations.
30 pages, 4 figures. v2: one reference added, minor revisions, accepted for publication in JHEP
References in corpus (2)
Cited by in corpus (25)
- QCD and strongly coupled gauge theories: challenges and perspectives
- 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
- Baryon and lepton number violation rates across the electroweak crossover
- Robust approach to thermal resummation: Standard Model meets a singlet
- Combining thermal resummation and gauge invariance for electroweak phase transition
- Precise WIMP Dark Matter Abundance and Standard Model Thermodynamics
- Four-loop pressure of massless O(N) scalar field theory
- Three-dimensional effective theories for the two Higgs doublet model at high temperature
- Pressure of the Standard Model Near the Electroweak Phase Transition
- The diagonal and off-diagonal quark number susceptibility of high temperature and finite density QCD
- Effects of the QCD Equation of State and Lepton Asymmetry on Primordial Gravitational Waves
- Equation of State for Cosmological Matter at and beyond QCD and Electroweak Eras
- The Electroweak Phase Transition in Ultra Minimal Technicolor
- Mesonic screening masses at high temperature and finite density
- Gravitational mass-shift effect in the Standard Model
- Cosmology from Strong Interactions
- Speed of sound in cosmological phase transitions and effect on gravitational waves
- Hard thermal contributions to phase transition observables at NNLO
- Pressure of the standard model