More Viable Parameter Space for Leptogenesis
arXiv:1401.3278 · doi:10.1103/PhysRevD.90.063522
Abstract
Lepton flavour asymmetries generated at the onset of the oscillations of sterile neutrinos with masses above the electroweak scale can be large enough to partly survive washout and to explain the baryon asymmetry of the Universe. This opens up new regions of parameter space, where Leptogenesis is viable within the type-I seesaw framework. In particular, we find it possible that the sterile neutrinos masses are substantially below 10^9 GeV, while not being degenerate. However, the required reheat temperature that is determined by the begin of the oscillations lies some orders of magnitude above the sterile neutrino mass-scale.
20 pages, journal version, explanations added
References in corpus (5)
- Leptogenesis
- Thermal production of relativistic Majorana neutrinos: Strong enhancement by multiple soft scattering
- Leptogenesis and Neutrino Oscillations in the Classically Conformal Standard Model with the Higgs Portal
- Baryogenesis through Neutrino Oscillations: A Unified Perspective
- Thermal right-handed neutrino production rate in the relativistic regime
Cited by in corpus (18)
- A facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case
- A White Paper on keV Sterile Neutrino Dark Matter
- Combining Experimental and Cosmological Constraints on Heavy Neutrinos
- Testing the low scale seesaw and leptogenesis
- The seesaw portal in testable models of neutrino masses
- ARS Leptogenesis
- Probing Leptogenesis at Future Colliders
- Probing leptogenesis with GeV-scale sterile neutrinos at LHCb and BELLE II
- Uniting low-scale leptogeneses
- Neutrinoless double decay and low scale leptogenesis
- Sterile Neutrino Dark Matter and Low Scale Leptogenesis from a Charged Scalar
- Initial condition for baryogenesis via neutrino oscillation
- Baryogenesis and Dark Matter from Freeze-In
- Thermal Leptogenesis in the Minimal Gauged Model
- Low-scale leptogenesis with flavour and CP symmetries
- Phenomenology of Baryogenesis from Lepton-Doublet Mixing
- Reconciling resonant leptogenesis and baryogenesis via neutrino oscillations
- How many new particles do we need after the Higgs boson?