Leptogenesis in the Universe
By C. S. Fong, E. Nardi, A. Riotto. 2012
161 citations recorded by the source corpus.
Leptogenesis is a class of scenarios in which the cosmic baryon asymmetry originates from an initial lepton asymmetry generated in the decays of heavy sterile neutrinos in the early Universe. We explain why leptogenesis is an appealing mechanism for baryogenesis. We review its motivations and the basic ingredients and describe subclasses of effects, like those of lepton flavours, spectator processes, scatterings, finite temperature corrections, the role of the heavier sterile neutrinos, and quantum corrections. We then address leptogenesis in supersymmetric scenarios, as well as some other popular variations of the basic leptogenesis framework.
Subfields: Artificial Intelligence, Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ed6a3a058cb27b324edbe444293cd5546e775eca
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In Artificial Intelligence
In Astronomy and Astrophysics
- M. Drewes
- The IceCube Collaboration
- Luca Visinelli
- L. Luzio
- E. Nardi
- Giovanni Signorelli
- L. Calibbi
- Maurizio Giannotti
In Nuclear and High Energy Physics
- Luca Visinelli
- L. Luzio
- E. Nardi
- M. Drewes
- The IceCube Collaboration
- Giovanni Signorelli
- L. Calibbi
- Maurizio Giannotti
Citations in the corpus
- The landscape of QCD axion models (2020, background): “The serious drawbacks of these two theories are that supersymmetry has not been found at the LHC, while the experimental verification of type-I seesaw leptogenesis remains well outside the reach of all current experiments [11–15].”
- The Phenomenology of Right Handed Neutrinos (2013, background): “The importance of flavour has been realized in [395] and [396–399] and meanwhile been studied by various authors, see [388, 389] for details and references.”
- Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU) (2014, background): “In addition, the determination of the NMH will influence the interpretation of non-oscillation experiments (neutrinoless double beta decay and beta decay) sensitive to the particle nature of the neutrino (Dirac vs Majorana) and/or its absolute mass [14], and will thus help to test popular see-saw ne”
- Charged Lepton Flavour Violation: An Experimental and Theoretical Introduction (2017, background): “(33) naively gives MR ∼ 1014 ÷ 1015 GeV for Yν ∼ O (1).”