It is shown that hypothetical neutrino-majoron coupling can suppress neutrino flavor oscillations in the early universe, in contrast to the usual weak interaction case. This reopens a window for a noticeable cosmological lepton asymmetry which is forbidden for the large mixing angle solution in the case of standard interactions of neutrinos
We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino fla...
We show that, if they exist, lepton number asymmetries ($$L_\alpha $$) of neutrino flavors should be...
We discuss the oscillations effects on neutrinos in the early Universe and update the cosmological c...
It is shown that hypothetical neutrino-majoron coupling can suppress neutrino flavor oscillations in...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
We investigate neutrino flavor transformation in the early universe in the presence of a lepton asym...
International audienceWhile the baryon asymmetry of the Universe is nowadays well measured bycosmolo...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
International audienceWhile the baryon asymmetry of the Universe is nowadays well measured bycosmolo...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
We explore charged lepton mixing and oscillations as a consequence of neutrino mixing in the early U...
Abstract We study three-flavor neutrino oscillations in the early universe in the presence of neutri...
It is well known that flavor oscillations in the early universe roughly equalize possible primordial...
We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino fla...
We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino fla...
We show that, if they exist, lepton number asymmetries ($$L_\alpha $$) of neutrino flavors should be...
We discuss the oscillations effects on neutrinos in the early Universe and update the cosmological c...
It is shown that hypothetical neutrino-majoron coupling can suppress neutrino flavor oscillations in...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
We investigate neutrino flavor transformation in the early universe in the presence of a lepton asym...
International audienceWhile the baryon asymmetry of the Universe is nowadays well measured bycosmolo...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
International audienceWhile the baryon asymmetry of the Universe is nowadays well measured bycosmolo...
While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, t...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
We explore charged lepton mixing and oscillations as a consequence of neutrino mixing in the early U...
Abstract We study three-flavor neutrino oscillations in the early universe in the presence of neutri...
It is well known that flavor oscillations in the early universe roughly equalize possible primordial...
We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino fla...
We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino fla...
We show that, if they exist, lepton number asymmetries ($$L_\alpha $$) of neutrino flavors should be...
We discuss the oscillations effects on neutrinos in the early Universe and update the cosmological c...