Add to ORKGA mechanism of radiatively generating neutrino masses is implemented in an SU(2)_L x U(1)_Y x SU(2)'_L x U(1)'_Y model, where the first and second families respect SU(2)_L x U(1)_Y while SU(2)'_L x U(1)'_Y is specific for the third family. The fourth neutrino, nu_s, that has a U(1)_Y x U(1)'_Y coupling joins in the model to induce neutrino mixings by additional interactions with e and mu. The phenomenologically consistent oscillation of nu_s - nu_e requires a dominated coupling of nu_s to e
A simple model to accomodate light sterile neutrinos naturally with large mixing with the usual neut...
We studied models of leptogenesis where three right-handed Majorana neutrinos are involved and the m...
Neutrino flavor mixing is explained within the recently proposed low-scale minimal linear seesaw mod...
e have constructed an $SU(3)_L \times U(1)_N$ gauge model utilizing an $U(1)_{L^\prime}$ symmetry, w...
We discuss the structure of the neutrino mass matrix as derived from a nonuniversal electroweak gaug...
It is shown that if small neutrino masses owe their origin to the conventional seesaw mechanism and ...
I review the various mechanisms for obtaining nonzero neutrino masses. I focus on the possibility of...
A simple unifying mass matrix is presented for the three active and one sterile neutrinos $\nu_e$, $...
金沢大学理工研究域数物科学系We consider the explanation of both data of the atmospheric neutrino and the solar neu...
Several neutrino experiments have reported results that are potentially inconsistent with our curren...
We consider the minimal extended seesaw model which can accommodate an eV scale sterile neutrino. Th...
The renormalization-group equation (RGE) approach to neutrino matter effects is further developed in...
It has been observed that simultaneous explanation of the solar and atmospheric neutrino deficits an...
Sterile neutrinos can be produced in the early universe via interactions with their active counterpa...
ABSTRACT: We investigate the neutrino masses and mixing patten in a version of the SU(3)c⊗SU(3)L⊗U(1...
A simple model to accomodate light sterile neutrinos naturally with large mixing with the usual neut...
We studied models of leptogenesis where three right-handed Majorana neutrinos are involved and the m...
Neutrino flavor mixing is explained within the recently proposed low-scale minimal linear seesaw mod...
e have constructed an $SU(3)_L \times U(1)_N$ gauge model utilizing an $U(1)_{L^\prime}$ symmetry, w...
We discuss the structure of the neutrino mass matrix as derived from a nonuniversal electroweak gaug...
It is shown that if small neutrino masses owe their origin to the conventional seesaw mechanism and ...
I review the various mechanisms for obtaining nonzero neutrino masses. I focus on the possibility of...
A simple unifying mass matrix is presented for the three active and one sterile neutrinos $\nu_e$, $...
金沢大学理工研究域数物科学系We consider the explanation of both data of the atmospheric neutrino and the solar neu...
Several neutrino experiments have reported results that are potentially inconsistent with our curren...
We consider the minimal extended seesaw model which can accommodate an eV scale sterile neutrino. Th...
The renormalization-group equation (RGE) approach to neutrino matter effects is further developed in...
It has been observed that simultaneous explanation of the solar and atmospheric neutrino deficits an...
Sterile neutrinos can be produced in the early universe via interactions with their active counterpa...
ABSTRACT: We investigate the neutrino masses and mixing patten in a version of the SU(3)c⊗SU(3)L⊗U(1...
A simple model to accomodate light sterile neutrinos naturally with large mixing with the usual neut...
We studied models of leptogenesis where three right-handed Majorana neutrinos are involved and the m...
Neutrino flavor mixing is explained within the recently proposed low-scale minimal linear seesaw mod...