The cosmological constant and Higgs mass with emergent gauge symmetries
arXiv:2004.05489 · doi:10.5506/APhysPolB.51.1251
Abstract
We discuss the Higgs mass and cosmological constant in the context of an emergent Standard Model, where the gauge symmetries "dissolve" in the extreme ultraviolet. In this scenario the cosmological constant scale is suppressed by power of the large scale of emergence and expected to be of similar size to neutrino masses. Cosmology constraints then give an anthropic upper bound on the Higgs mass.
16 pages, 4 figures, presented at the XXVI Cracow Epiphany Conference on LHC Physics: Standard Model and Beyond, January 7-10 2020
Cited by in corpus (5)
- Renormalizing the vacuum energy in cosmological spacetime: implications for the cosmological constant problem
- The Higgs boson -- its implications and prospects for future discoveries
- Emergent gauge symmetries -- making symmetry as well as breaking it
- Is "Dark Energy" a Quantum Vacuum Energy?
- The cosmological constant and scale hierarchies with emergent gauge symmetries