We determine the restrictions imposed by primordial nucleosynthesis upon a heavy tau neutrino, in the presence of ~, ~ annihilations into majorons, as expected in a wide class of particle physics models of neutrino mass. We determine the equivalent umber of light neutrino species Neq as a function of m,, and the v~-vr-majoron coupling. We show that for theoretically plausible g values ~> 10-4 present nucleosynthesis observations can not rule out v ~ masses in the MeV range. Moreover, these models give Neq ~< 3 in the v ~ mass region 1-10 MeV, for very reasonable values of g/> 3 × 10-4. The evasion of the cosmological limits brings new interest to the improvement of the present laboratory limit on the ~, ~ mass which can be achieved...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...
The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experim...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...
We determine the restrictions imposed by primordial nucleosynthesis upon a heavy tau neutrino, in th...
The primordial abundance of long-lived heavy Majorana neutrinos is calculated from the full Boltzman...
Sterile massive neutrinos are a natural extension of the standard model of elementary particles. The...
. A massive long-lived ø neutrino in the MeV regime modifies the primordial light-element abundances...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between v(...
Recent experimental results, together with a cosmological argument concerning the survival of primor...
Recent experimental results, together with a cosmological argument concerning the survival of primor...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We determine the upper limit on the mass of the lightest neutrino from the most robust recent cosmol...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...
The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experim...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...
We determine the restrictions imposed by primordial nucleosynthesis upon a heavy tau neutrino, in th...
The primordial abundance of long-lived heavy Majorana neutrinos is calculated from the full Boltzman...
Sterile massive neutrinos are a natural extension of the standard model of elementary particles. The...
. A massive long-lived ø neutrino in the MeV regime modifies the primordial light-element abundances...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between v(...
Recent experimental results, together with a cosmological argument concerning the survival of primor...
Recent experimental results, together with a cosmological argument concerning the survival of primor...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We compute the nucleosynthesis bounds on the masses of stable Dirac and Majorana neutrinos by solvin...
We determine the upper limit on the mass of the lightest neutrino from the most robust recent cosmol...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...
The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experim...
The data on atmospheric neutrinos can be explained assuming the existence of oscillations between mu...