Anish Ghoshal
Superradiant leptogenesis
Ghoshal, Anish; Perez-Gonzalez, Yuber F.; Turner, Jessica
Authors
Yuber Perez Gonzalez yuber.f.perez-gonzalez@durham.ac.uk
Post Doctoral Research Associate
Jessica Turner jessica.turner@durham.ac.uk
Assistant Professor
Abstract
We investigate how superradiance affects the generation of baryon asymmetry in a universe with rotating primordial black holes, considering a scenario where a scalar boson is coupled to the heavy right-handed neutrinos. We identify the regions of the parameter space where the scalar production is enhanced due to superradiance. This enhancement, coupled with the subsequent decay of the scalar into right handed neutrinos, results in the non-thermal creation of lepton asymmetry. We show that successful leptogenesis is achieved for masses of primordial black holes in the range of order O(0.1 g) − O(10 g) and the lightest of the heavy neutrino masses, MN ~ O(1012) GeV. Consequently, regions of the parameter space, which in the case of Schwarzchild PBHs were incompatible with viable leptogenesis, can produce the observed matter-antimatter asymmetry.
Citation
Ghoshal, A., Perez-Gonzalez, Y. F., & Turner, J. (2024). Superradiant leptogenesis. Journal of High Energy Physics, 2024(2), Article 113. https://doi.org/10.1007/jhep02%282024%29113
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 27, 2024 |
Online Publication Date | Feb 15, 2024 |
Publication Date | Feb 15, 2024 |
Deposit Date | Mar 18, 2024 |
Publicly Available Date | Mar 18, 2024 |
Journal | Journal of High Energy Physics |
Print ISSN | 1126-6708 |
Publisher | Scuola Internazionale Superiore di Studi Avanzati (SISSA) |
Peer Reviewed | Peer Reviewed |
Volume | 2024 |
Issue | 2 |
Article Number | 113 |
DOI | https://doi.org/10.1007/jhep02%282024%29113 |
Keywords | Sterile or Heavy Neutrinos, Baryo-and Leptogenesis, Cosmology of Theories BSM, Baryon/Lepton Number Violation |
Public URL | https://durham-repository.worktribe.com/output/2275914 |
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Copyright Statement
Open Access. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
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