Neutrino masses and mixings are analyzed in terms of left-handed fields and a 6x6 complex symmetric mass matrix whose singular values are the neutrino masses. An angle theta_nu characterizes the kind of the neutrinos, with theta_nu = 0 for Dirac neutrinos and theta_nu = pi/2 for Majorana neutrinos. If theta_nu = 0, then baryon-minus-lepton number is conserved. When theta_nu is approximately zero, the six neutrino masses coalesce into three nearly degenerate pairs. Thus the smallness of the differences in neutrino masses exhibited in the solar and atmospheric neutrino experiments and the stringent limits on neutrinoless double-beta decay are naturally explained if B-L is approximately conserved and neutrinos are nearly Dirac fermions. If one...
After a brief introduction to neutrino mass via the see-saw model I discuss neutrino mixing and osci...
In the framework of a left-right model containing mirror fermions with gauge group SU(3)(C) circle t...
After briefly reviewing how the symmetries of the Standard Model (SM) are affected by neutrino masse...
We show that in theories that reduce, at the Fermi scale, to an extension of the standard model with...
We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense...
We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense...
In spite of the general belief that neutrinos are Majorana particles, their character should be reve...
We propose a novel theoretical understanding of neutrino masses and mixings, which is attributed to ...
Recent neutrino experiments have made very significant progresses and our knowledge of neutrino mass...
In this talk I review our present knowledge on neutrino masses and mixing as well as the expectation...
Motivated by cosmological considerations, and by the atmospheric and solar neutrino flux deficits, w...
AbstractWe study the possible structure of the neutrino mass matrix taking into consideration the so...
The combined requirements, of (i) a natural solution to the fermion mass hierarchy problem and (ii) ...
In spite of enormous experimental progress in determination of the neutrino parameters, theory of ne...
Two schemes of mixing of four massive neutrinos with two close neutrino masses separated by a gap of...
After a brief introduction to neutrino mass via the see-saw model I discuss neutrino mixing and osci...
In the framework of a left-right model containing mirror fermions with gauge group SU(3)(C) circle t...
After briefly reviewing how the symmetries of the Standard Model (SM) are affected by neutrino masse...
We show that in theories that reduce, at the Fermi scale, to an extension of the standard model with...
We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense...
We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense...
In spite of the general belief that neutrinos are Majorana particles, their character should be reve...
We propose a novel theoretical understanding of neutrino masses and mixings, which is attributed to ...
Recent neutrino experiments have made very significant progresses and our knowledge of neutrino mass...
In this talk I review our present knowledge on neutrino masses and mixing as well as the expectation...
Motivated by cosmological considerations, and by the atmospheric and solar neutrino flux deficits, w...
AbstractWe study the possible structure of the neutrino mass matrix taking into consideration the so...
The combined requirements, of (i) a natural solution to the fermion mass hierarchy problem and (ii) ...
In spite of enormous experimental progress in determination of the neutrino parameters, theory of ne...
Two schemes of mixing of four massive neutrinos with two close neutrino masses separated by a gap of...
After a brief introduction to neutrino mass via the see-saw model I discuss neutrino mixing and osci...
In the framework of a left-right model containing mirror fermions with gauge group SU(3)(C) circle t...
After briefly reviewing how the symmetries of the Standard Model (SM) are affected by neutrino masse...