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Leptogenesis (0802.2962v3)

Published 20 Feb 2008 in hep-ph

Abstract: Leptogenesis is a class of scenarios where the baryon asymmetry of the Universe is produced from a lepton asymmetry generated in the decays of a heavy sterile neutrino. We explain the motivation for leptogenesis. We review the basic mechanism, and describe subclasses of models. We then focus on recent developments in the understanding of leptogenesis: finite temperature effects, spectator processes, and in particular the significance of flavor physics.

Citations (718)
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Summary

  • The paper establishes that heavy Majorana neutrino decays within the seesaw framework generate CP asymmetry crucial for initiating thermal leptogenesis.
  • It employs Boltzmann equations with flavor effects to model the dynamics of particle decays, inverse decays, and scatterings.
  • The research constrains neutrino mass bounds and reheat temperature, guiding future experiments and theoretical models in particle physics.

An Overview of Thermal Leptogenesis and Its Implications for the Baryon Asymmetry of the Universe

The origin of the baryon asymmetry of the Universe (BAU) remains one of the most profound questions in cosmology and particle physics. The concept of leptogenesis offers a compelling framework by which this asymmetry could be generated via the dynamics of neutrino physics. The paper under review explores the theoretical mechanisms of thermal leptogenesis, linking it closely with the seesaw model of neutrino masses.

The Seesaw Mechanism and Leptogenesis

The seesaw mechanism stands as a robust theoretical model for explaining the smallness of neutrino masses. It introduces heavy Majorana neutrinos which, when integrated into the Standard Model, break lepton number symmetry and furnish a natural explanation for the observed light neutrino masses. The introduction of these heavy neutrinos not only serves to explain neutrino masses but also leads to the possibility of generating a lepton asymmetry in the early Universe—a process termed leptogenesis—which can be converted into a baryon asymmetry through electroweak sphaleron processes.

Thermal Leptogenesis: Dynamics and CP Asymmetry

At the core of thermal leptogenesis is the out-of-equilibrium decay of these heavy neutrinos in the early Universe. The paper details the dynamics of this process, emphasizing the role of CP asymmetry in their decay channels. This asymmetry is a result of the interference between tree-level and one-loop decay diagrams of the heavy neutrinos, leading to a net excess of leptons over anti-leptons.

Boltzmann Equations and Flavour Effects

To quantitatively describe the evolution of particle densities and asymmetries, the paper employs Boltzmann equations. These equations account for various processes including decays, inverse decays, and scatterings. A significant advancement covered by the paper is the inclusion of flavour effects. Previously, leptogenesis calculations often ignored the flavour composition of leptons, but this paper demonstrates that accounting for these effects can significantly affect the washout processes and the resulting baryon asymmetry.

Implications and Model Constraints

The CP violation needed for leptogenesis to work successfully also places constraints on the mass and properties of the heavy neutrinos. A particularly intriguing aspect discussed is the bound on the mass of the lightest heavy neutrino, which has implications for the reheat temperature of the Universe. This is especially pertinent in supersymmetric models where thermal effects and the potential for gravitinogenesis place additional constraints on the parameter space.

Future Directions and Challenges

While the paper makes substantial progress in deepening our understanding of leptogenesis, several challenges remain. The precise nature of CP violation and its measurability at low-energy experiments remains an open question. Furthermore, the complexity of modelling all relevant thermal effects and spectator processes invites future work to refine these calculations.

Conclusion

Leptogenesis continues to be a promising framework for explaining the BAU. This paper provides a comprehensive exploration of the necessary theoretical machinery, highlighting both the successes and the hurdles that remain. The potential intersection of leptogenesis with neutrino experiments and high-energy collider physics offers a pathway to uncovering the mystery of matter-antimatter asymmetry. As our theoretical understanding deepens, so too does the experimental challenge of verifying these predictions, making leptogenesis a central theme in the quest to understand our Universe's fundamental workings.

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