Baryogenesis from a right-handed neutrino condensate
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Baryogenesis from a right-handed neutrino condensate

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Baryogenesis from a right-handed neutrino condensate

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Barenboim Szuchman, Gabriela Alejandra Perfil; Rasero Daparte, Javier
Aquest document és un/a article, creat/da en: 2011
We show that the baryon asymmetry of the Universe can be generated by a strongly coupled right handed neutrino condensate which also drives inflation. The resulting model has only a small number of parameters, which completely determine not only the baryon asymmetry of the Universe and the mass of the right handed neutrino but also the inflationary phase. This feature allows us to make predictions that will be tested by current and planned experiments. As compared to the usual approach our dynamical framework is both economical and predictive.

    Barenboim Szuchman, Gabriela Alejandra Rasero Daparte, Javier 2011 Baryogenesis from a right-handed neutrino condensate Journal of High Energy Physics 2011 3 097
http://dx.doi.org/10.1007/JHEP03(2011)097
distribuït sota llicència Creative Commons de Reconeixement-NoComercial 3.0 No adaptada

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