Vacuum stability of the type II seesaw leptogenesis from inflation
arXiv:2208.11336 · doi:10.1103/PhysRevD.107.015021
Abstract
Recently it has been found that introducing a triplet Higgs to the standard model could provide a feasible leptogenesis to generate the baryon asymmetry of our universe, providing that the inflation is driven by the mixing state of the triplet Higgs and SM Higgs. In this work, we survey the viable parameter space satisfying the vacuum stability and perturbativity in this model. We find that the introduction of the triplet Higgs would also ameliorate the problem of the Higgs vacuum instability. We present two representative parameter regions where the origin of neutrino masses, baryon asymmetry of the universe as well as inflation can be explained while keeping consistent with the condition of vacuum stability and perturbativity.
References in corpus (29)
- Investigating the near-criticality of the Higgs boson
- SARAH 4: A tool for (not only SUSY) model builders
- Baryogenesis from Flat Directions of the Supersymmetric Standard Model
- Constraining f(R) Gravity as a Scalar Tensor Theory
- The Higgs Potential in the Type II Seesaw Model
- Unitarizing Higgs Inflation
- Chaotic Inflation and Baryogenesis in Supergravity
- Higgs Scalaron Mixed Inflation
- Vacuum Stability, Perturbativity, EWPD and Higgs-to-diphoton rate in Type II Seesaw Models
- Scalaron the healer: removing the strong-coupling in the Higgs- and Higgs-dilaton inflations
- Higgs Portal Inflation
- Preheating after Higgs Inflation: Self-Resonance and Gauge boson production
- Distinguishing between R^2-inflation and Higgs-inflation
- Quintessence Saves Higgs Instability
- Revisiting Type-II see-saw: Present Limits and Future Prospects at LHC
- Consistency of the triplet seesaw model revisited
- Dynamical Emergence of Scalaron in Higgs Inflation
- Light inflaton completing Higgs inflation
- Higgs Inflation as Nonlinear Sigma Model and Scalaron as its -meson
- Affleck-Dine Leptogenesis from Higgs Inflation
- Vacuum stability and naturalness in type-II seesaw
- Type II Seesaw Leptogenesis
- Affleck-Dine Baryogenesis with Observable Neutron-Anti-Neutron Oscillation
- Affleck-Dine Sneutrino Inflation
- Vacuum Stability Conditions for Higgs Potentials with Triplets
- Affleck-Dine leptogenesis with triplet Higgs
- Neutrino Mass from Affleck-Dine Leptogenesis and WIMP Dark Matter
- Higgs Inflation, Vacuum Stability, and Leptogenesis
- Pendulum Leptogenesis