Explanation for why the early universe was stable and dominated by the standard model
From MaRDI portal
Publication:5027089
DOI10.1088/1475-7516/2020/12/025zbMath1484.83126arXiv1911.04648OpenAlexW3113023114MaRDI QIDQ5027089
Publication date: 3 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1911.04648
inflationcosmology of theories beyond the SMphysics of the early universeparticle physics-cosmology connection
Unified quantum theories (81V22) Relativistic cosmology (83F05) Nuclear physics (81V35) Quantization of the gravitational field (83C45) Renormalization group methods applied to problems in quantum field theory (81T17) Classical and relativistic thermodynamics (80A10)
Related Items
The effective Higgs potential and vacuum decay in Starobinsky inflation ⋮ Vacuum decay constraints on the Higgs curvature coupling from inflation
Cites Work
- A Monte Carlo exploration of threefold base geometries for 4d F-theory vacua
- (Higgs) vacuum decay during inflation
- Scalaron the healer: removing the strong-coupling in the Higgs- and Higgs-Dilaton inflations
- Dark matter scattering cross Section and dynamics in dark Yang-Mills theory
- The cosmological higgstory of the vacuum instability
- Electroweak vacuum instability and renormalized Higgs field vacuum fluctuations in the inflationary universe
- Lattice formulation of axion inflation. Application to preheating
- On the metastability of the Standard Model vacuum
- Completion of standard-like embeddings