The compatibility of a recent possible explanation of the solar-neutrino puzzle and the result of Boris et al. on limits on neutrino mass is discussed. It is shown that if the electron and muon Majorana neutrinos combine to form a pseudo-Dirac particle of mass ~35 eV, then the radiative corrections will generate a mass-square difference 3×10−5 eV, which explains why Davis and his collaborators find fewer solar neutrinos than predicted. This idea can be naturally embedded in superstring theories
We analyze the status of the exotic solutions to the solar neutrino problem, i.e., those solutions b...
The Dirac masses of neutrinos can exhibit a strong hierarchy even if the Majorana masses of the righ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...
AbstractWe study the pseudo-Dirac mixing of left- and right-handed neutrinos in the case where the M...
A simple extension of the standard model is proposed in which all the three generations of neutrinos...
Mikheyev and Smirnov have shown that the interactions of neutrinos with matter can result in the con...
The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle a...
In the standard model of particle physics, neutrinos are necessarily massless. How-ever, recent expe...
We calculate a relative neutrino mass difference of Delta m / m = 6 10^-9 at the one loop level in a...
The minimally extended standard model of particle physics contains three right handed or sterile neu...
The study of solar neutrinos has given a fundamental contribution both to astroparticle and to eleme...
We propose a new mechanism to generate a 17 keV pseudo-Dirac neutrino naturally without subscribing ...
We show that all the available experimental information involving neutrinos can be accounted for wit...
What can we learn from solar neutrino observations? Is there any solution to the solar neutrino anom...
The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal os...
We analyze the status of the exotic solutions to the solar neutrino problem, i.e., those solutions b...
The Dirac masses of neutrinos can exhibit a strong hierarchy even if the Majorana masses of the righ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...
AbstractWe study the pseudo-Dirac mixing of left- and right-handed neutrinos in the case where the M...
A simple extension of the standard model is proposed in which all the three generations of neutrinos...
Mikheyev and Smirnov have shown that the interactions of neutrinos with matter can result in the con...
The study of solar neutrinos has given since ever a fundamental contribution both to astroparticle a...
In the standard model of particle physics, neutrinos are necessarily massless. How-ever, recent expe...
We calculate a relative neutrino mass difference of Delta m / m = 6 10^-9 at the one loop level in a...
The minimally extended standard model of particle physics contains three right handed or sterile neu...
The study of solar neutrinos has given a fundamental contribution both to astroparticle and to eleme...
We propose a new mechanism to generate a 17 keV pseudo-Dirac neutrino naturally without subscribing ...
We show that all the available experimental information involving neutrinos can be accounted for wit...
What can we learn from solar neutrino observations? Is there any solution to the solar neutrino anom...
The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal os...
We analyze the status of the exotic solutions to the solar neutrino problem, i.e., those solutions b...
The Dirac masses of neutrinos can exhibit a strong hierarchy even if the Majorana masses of the righ...
The present status of the solar neutrino problem is reviewed. The strongest motivation for new neutr...