Leptogenesis with perturbations in type-II and type-III seesaw models
arXiv:2503.02936 · doi:10.1140/epjc/s10052-025-14277-9
Abstract
Density perturbations have recently been shown to lead to a novel effect in the freeze-out of heavy particles called "acoustically driven freeze-out." This leads to an enhancement in the yield in standard leptogenesis. We extend this calculation to include washout processes in type-I leptogenesis and the Sommerfeld-enhanced gauge annihilations in type-II and type-III leptogenesis. These CP conserving gauge annihilations suppress the yield of heavy particles sourcing the asymmetry. We show the acoustically driven freeze-out leads to novel enhancements in the baryon asymmetry in type-II and type-III leptogenesis, already in the weak washout regime, in contrast with type-I leptogenesis.
9 pages, 3 figures, comments begrudgingly welcomed. v2: small corrections, references added. v3: minor comments added
References in corpus (54)
- Observation of electron-antineutrino disappearance at Daya Bay
- Observation of Reactor Electron Antineutrino Disappearance in the RENO Experiment
- Investigating the near-criticality of the Higgs boson
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- A lower bound on the right-handed neutrino mass from leptogenesis
- Resonant Leptogenesis
- Leptogenesis for Pedestrians
- Towards a complete theory of thermal leptogenesis in the SM and MSSM
- Neutrino Masses and Leptogenesis with Heavy Higgs Triplets
- The importance of flavor in leptogenesis
- Flavour Issues in Leptogenesis
- Flavour Matters in Leptogenesis
- Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum
- The Neutrino Mass Window for Baryogenesis
- Constraints on neutrino masses from leptogenesis models
- CMB at 2x2 order: the dissipation of primordial acoustic waves and the observable part of the associated energy release
- Consequences of Triplet Seesaw for Leptogenesis
- Type II Leptogenesis and the Neutrino Mass Scale
- Dynamical generation of the weak and Dark Matter scale
- Leptogenesis at the TeV scale
- Silk damping at a redshift of a billion: a new limit on small-scale adiabatic perturbations
- Spectator processes and baryogenesis
- Strong gravitational radiation from a simple dark matter model
- Gravitational Waves from First-Order Phase Transitions: LIGO as a Window to Unexplored Seesaw Scales
- Super-cool Dark Matter
- On Higgs and sphaleron effects during the leptogenesis era
- Efficiency and maximal CP-asymmetry of scalar triplet leptogenesis
- Revisiting constraints on small scale perturbations from big-bang nucleosynthesis
- The Gravitational Wave Spectrum from Cosmological B-L Breaking
- Must Cosmological Perturbations Remain Non-Adiabatic After Multi-Field Inflation?
- Conformal model for gravitational waves and dark matter: A status update
- Spontaneous B-L Breaking as the Origin of the Hot Early Universe
- Towards leptogenesis at NLO: the right-handed neutrino interaction rate
- String Fragmentation in Supercooled Confinement and Implications for Dark Matter
- Low-scale leptogenesis and soft supersymmetry breaking
- Leptogenesis triggered by a first-order phase transition
- Leptogenesis: beyond the minimal type I seesaw scenario
- Supercool Composite Dark Matter Beyond 100 TeV
- Sommerfeld corrections to type-II and III leptogenesis
- Reheating the Universe Once More: The Dissipation of Acoustic Waves as a Novel Probe of Primordial Inhomogeneities on Even Smaller Scales
- Cosmological Perturbations at Second Order and Recombination Perturbed
- Type-I Seesaw as the Common Origin of Neutrino Mass, Baryon Asymmetry, and the Electroweak Scale
- Constraining first-order phase transitions with curvature perturbations
- The Neutrino Option
- Conformal Realization of the Neutrino Option
- Leptogenesis with a dynamical seesaw scale
- Strong Supercooling as a Consequence of Renormalization Group Consistency
- Examining the neutrino option
- Leptogenesis in the Neutrino Option
- Freeze-in Dark Matter Perturbations are Adiabatic
- Impact of freeze-in on dark matter isocurvature
- Dark Matter from freeze-in and its inhomogeneities
- Baryogenesis via Leptogenesis in an inhomogeneous universe
- Dark Matter Isocurvature from Curvature