Abstract
Cosmological considerations imply that the Weinberg-Salam Higgs boson mass ${m}_{\mathrm{H}}\ensuremath{\gtrsim}9$ GeV. If this bound were violated, the symmetry-breaking phase transition would occur only after extreme supercooling, resulting in too high a ratio of entropy to baryon number.
Keywords
Affiliated Institutions
Related Publications
Weak interactions at very high energies: The role of the Higgs-boson mass
We give an $S$-matrix-theoretic demonstration that if the Higgs-boson mass exceeds ${M}_{c}={(8\ensuremath{\pi}\frac{\sqrt{2}}{3}{G}_{F})}^{\frac{1}{2}}$, parital-wave unitarity...
Conservative constraints on early cosmology with MONTE PYTHON
Models for the latest stages of the cosmological evolution rely on a less solid theoretical and observational ground than the description of earlier stages like BBN and recombin...
Publication Info
- Year
- 1980
- Type
- article
- Volume
- 45
- Issue
- 14
- Pages
- 1131-1134
- Citations
- 91
- Access
- Closed
External Links
Social Impact
Social media, news, blog, policy document mentions
Citation Metrics
Cite This
Identifiers
- DOI
- 10.1103/physrevlett.45.1131