Linear seesaw leptogenesis before/after electroweak symmetry breaking
arXiv:2509.14524 · doi:10.1103/85vc-x819
Abstract
The linear seesaw (LSS) model provides a natural framework for generating small neutrino masses at low energy scales, thereby offering promising testability prospects. However, in generic LSS models, the exact mass degeneracy (before the electroweak symmetry breaking) between the two sterile neutrinos that form a Dirac pair precludes the generation of CP asymmetries from their interplay, posing a significant challenge to explaining the observed baryon (or lepton) asymmetry of the Universe via the leptogenesis mechanism. In this work, we explore two well-motivated approaches to generate a suitable mass splitting for the two sterile neutrinos that form a Dirac pair, and consequently naturally realize a resonantly enhanced generation of baryon (and lepton) asymmetry. First, we demonstrate that the renormalization group evolution effects can naturally induce the desired mass splitting for the sterile neutrinos, resulting in a successful generation of the observed baryon asymmetry of the Universe. Second, motivated by the recent result from the EMPRESS collaboration that indicates the possible existence of a large lepton asymmetry of the Universe, we explore the possibility that a large lepton asymmetry might naturally follow from the electroweak symmetry breaking which automatically induces the desired mass splitting for the sterile neutrinos.
19 pages,6 figures, version accepted for publication in PRD
References in corpus (38)
- In the Realm of the Hubble tension a Review of Solutions
- Oscillating neutrinos and mu --> e, gamma
- Leptogenesis
- The MSM, Dark Matter and Baryon Asymmetry of the Universe
- A lower bound on the right-handed neutrino mass from leptogenesis
- Resonant Leptogenesis
- Leptogenesis for Pedestrians
- The MSM, Dark Matter and Neutrino Masses
- Leptogenesis as the origin of matter
- The importance of flavor in leptogenesis
- Flavour Issues in Leptogenesis
- Novel Supersymmetric SO(10) Seesaw Mechanism
- The Sphaleron Rate in the Minimal Standard Model
- NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations
- Flavor structures of charged fermions and massive neutrinos
- Baryogenesis from the weak scale to the grand unification scale
- Lepton flavor violation and non-unitary lepton mixing in low-scale type-I seesaw
- EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension
- Large lepton asymmetry from Q-balls
- Pseudo-Dirac Scenario for Neutrino Oscillations
- Reconciling leptogenesis with observable mu --> e gamma rates
- Indications for a Nonzero Lepton Asymmetry from Extremely Metal-Poor Galaxies
- Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
- ULYSSES: Universal LeptogeneSiS Equation Solver
- Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology
- Lepton Asymmetric Universe
- Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
- Hubble tension in lepton asymmetric cosmology with an extra radiation
- Constraints on primordial lepton asymmetries with full neutrino transport
- Natural Seesaw and Leptogenesis from Hybrid of High-Scale Type I and TeV-Scale Inverse
- Large Neutrino Asymmetry from TeV Scale Leptogenesis
- Leptoflavorgenesis: baryon asymmetry of the Universe from lepton flavor violation
- HNL mass degeneracy: implications for low-scale seesaws, LNV at colliders and leptogenesis
- A full parametrization of the active-sterile flavor mixing matrix in the inverse or linear seesaw scenario of massive neutrinos
- Neutrino Anarchy and Renormalization Group Evolution
- Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
- Purely flavored leptogenesis from a sudden mass gain of right-handed neutrinos
- Low scale leptogenesis under neutrino - reflection symmetry