Academic literature on the topic 'Resonant leptogenesis'

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Journal articles on the topic "Resonant leptogenesis"

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Pilaftsis, Apostolos, and Thomas E. J. Underwood. "Resonant leptogenesis." Nuclear Physics B 692, no. 3 (2004): 303–45. http://dx.doi.org/10.1016/j.nuclphysb.2004.05.029.

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Simone, Andrea De, and Antonio Riotto. "On resonant leptogenesis." Journal of Cosmology and Astroparticle Physics 2007, no. 08 (2007): 013. http://dx.doi.org/10.1088/1475-7516/2007/08/013.

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Dev, P. S. B., M. Garny, J. Klaric, P. Millington, and D. Teresi. "Resonant enhancement in leptogenesis." International Journal of Modern Physics A 33, no. 05n06 (2018): 1842003. http://dx.doi.org/10.1142/s0217751x18420034.

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Vanilla leptogenesis within the type I seesaw framework requires the mass scale of the right-handed neutrinos to be above [Formula: see text] GeV. This lower bound can be avoided if at least two of the sterile states are almost mass degenerate, which leads to an enhancement of the decay asymmetry. Leptogenesis models that can be tested in current and upcoming experiments often rely on this resonant enhancement, and a systematic and consistent description is therefore necessary for phenomenological applications. In this paper, we give an overview of different methods that have been used to stud
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Kashiwase, Shoichi, Hiroshi Okada, Yuta Orikasa, and Takashi Toma. "Two loop neutrino model with dark matter and leptogenesis." International Journal of Modern Physics A 31, no. 20n21 (2016): 1650121. http://dx.doi.org/10.1142/s0217751x16501219.

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In this paper, we study a two-loop induced radiative neutrino model at TeV scale with global [Formula: see text] symmetry, in which we analyze dark matter and resonant leptogenesis. The model includes two kinds of dark matter candidates. We discuss what kind of dark matter can satisfy the observed relic density as well as the current direct detection bound, and be simultaneously compatible with the leptogenesis. We also discuss whether our resonant leptogenesis can be differentiated from the other scenarios at TeV scale or not.
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Dev, P. S. Bhupal, Peter Millington, Apostolos Pilaftsis, and Daniele Teresi. "Flavour Covariant Formalism for Resonant Leptogenesis." Nuclear and Particle Physics Proceedings 273-275 (April 2016): 268–74. http://dx.doi.org/10.1016/j.nuclphysbps.2015.09.037.

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Anisimov, A., A. Broncano, and M. Plümacher. "The CP-asymmetry in resonant leptogenesis." Nuclear Physics B 737, no. 1-2 (2006): 176–89. http://dx.doi.org/10.1016/j.nuclphysb.2006.01.003.

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Garbrecht, Björn, Florian Gautier, and Juraj Klaric. "Strong washout approximation to resonant leptogenesis." Journal of Cosmology and Astroparticle Physics 2014, no. 09 (2014): 033. http://dx.doi.org/10.1088/1475-7516/2014/09/033.

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Zhang, Jue, and Shun Zhou. "Neutrinos and cosmological matter–antimatter asymmetry: A minimal seesaw with Frampton–Glashow–Yanagida ansatz." International Journal of Modern Physics A 32, no. 16 (2017): 1742004. http://dx.doi.org/10.1142/s0217751x17420040.

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In light of the latest neutrino data, we revisit a minimal seesaw model with the Frampton–Glashow–Yanagida ansatz. Renormalization-group running effects on neutrino masses and flavor mixing parameters are discussed and found to essentially have no impact on testing such a minimal scenario in low-energy neutrino experiments. However, since renormalization-group running can modify neutrino mixing parameters at high energies, it does affect the leptogenesis mechanism, which is responsible for the observed matter–antimatter asymmetry in our Universe. Furthermore, to ease the conflict between the n
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Granelli, A., K. Moffat, and S. T. Petcov. "Flavoured resonant leptogenesis at sub-TeV scales." Nuclear Physics B 973 (December 2021): 115597. http://dx.doi.org/10.1016/j.nuclphysb.2021.115597.

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Hambye, Thomas, John March-Russell, and Stephen M. West. "TeV scale resonant leptogenesis from supersymmetry breaking." Journal of High Energy Physics 2004, no. 07 (2004): 070. http://dx.doi.org/10.1088/1126-6708/2004/07/070.

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Dissertations / Theses on the topic "Resonant leptogenesis"

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Faure, Rémi. "Neutrinos, cosmological phase transitions and the matter-antimatter asymmetry of the Universe." Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPASP081.

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L'asymétrie entre matière et antimatière est un problème non résolu de la cosmologie. Une approche populaire pour l'expliquer est la leptogénèse avec des neutrinos stériles, qui sont des particules motivées expérimentalement pour expliquer les masses des neutrinos actifs du Modèle Standard. Il est possible d'inclure dans les scénarios de leptogénèse une transition de phase cosmologique qui donne leur masse aux neutrinos stériles. Cette idée est intéressante phénoménologiquement, car une transition de phase produit des ondes gravitationnelles pouvant être détectées. À la température de la trans
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Book chapters on the topic "Resonant leptogenesis"

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Racker, J. "Non-resonant leptogenesis in seesaw models with an almost conserved B − L." In SSP 2012. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-6485-9_9.

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Conference papers on the topic "Resonant leptogenesis"

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Pilaftsis, Apostolos, Pablo Candia da Silva, Dimitrios Karamitros, and Thomas McKelvey. "Tri-Resonant Leptogenesis." In Corfu Summer Institute 2022 "School and Workshops on Elementary Particle Physics and Gravity". Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.436.0036.

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PILAFTSIS, A. "PHENOMENOLOGICAL IMPLICATIONS OF RESONANT LEPTOGENESIS." In Proceedings of the 10th International Symposium. World Scientific Publishing Company, 2005. http://dx.doi.org/10.1142/9789812701756_0044.

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Deppisch, Frank F., and Apostolos Pilaftsis. "Minimal resonant leptogenesis and lepton flavour violation." In GUT2012. AIP, 2012. http://dx.doi.org/10.1063/1.4742094.

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CAMPBELL, BRUCE A., and DAVID W. MAYBURY. "LEPTOGENESIS FROM PARAMETRIC RESONANCE." In Proceedings of the 20th Lake Louise Winter Institute. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812774422_0031.

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