We point out the simple reversibility between the fundamental neutrino mixing parameters in vacuum and their effective counterparts in matter. The former can therefore be expressed in terms of the latter, allowing more straightforward extraction of the genuine lepton mixing quantities from a variety of long-baseline neutrino oscillation experiments. In addition to the parametrization-independent results, we present the formulas based on the standard parametrization of the lepton flavor mixing matrix and give a typical numerical illustration
We propose a phenomenological model of lepton mixing and CP violation based on the flavor democracy ...
We provide a complete answer to the following question: what are the flavour groups and representat...
We show that the observed pattern for neutrino mixing arises naturally if neutrinos are composites o...
AbstractWe derive a new set of sum rules between the neutrino mass and mixing parameters in vacuum a...
We consider the case that the solar neutrino deficit is due to the vacuum oscillation. The lepton ma...
Recent atmospheric neutrino data at Super-Kamiokande suggest the large flavor mixing of neutrinos. M...
We determine the elements of the leptonic mixing matrix, without assuming unitarity, combining data ...
AbstractWe present the generic formulas to calculate the ratios of neutrino masses and the Majorana ...
Implications of a simple model for the mass generation of leptons are studied, in particular for the...
The measurement of the charged-current 8B solar neutrino reaction on deuterium at the Sudbury Neutri...
The search for possible mixing patterns of charged leptons and neutrinos is important to get clues o...
We explore some important implications of the KamLAND measurment on the lepton flavor mixing matrix ...
We introduce a simple flavor symmetry breaking scheme, in which charged lepton masses have a strong ...
Recently, many authors showed that if the solar and atmospheric neutrino data are both described by ...
We borrow the general idea of renormalization-group equations (RGEs) to understand how neutrino mass...
We propose a phenomenological model of lepton mixing and CP violation based on the flavor democracy ...
We provide a complete answer to the following question: what are the flavour groups and representat...
We show that the observed pattern for neutrino mixing arises naturally if neutrinos are composites o...
AbstractWe derive a new set of sum rules between the neutrino mass and mixing parameters in vacuum a...
We consider the case that the solar neutrino deficit is due to the vacuum oscillation. The lepton ma...
Recent atmospheric neutrino data at Super-Kamiokande suggest the large flavor mixing of neutrinos. M...
We determine the elements of the leptonic mixing matrix, without assuming unitarity, combining data ...
AbstractWe present the generic formulas to calculate the ratios of neutrino masses and the Majorana ...
Implications of a simple model for the mass generation of leptons are studied, in particular for the...
The measurement of the charged-current 8B solar neutrino reaction on deuterium at the Sudbury Neutri...
The search for possible mixing patterns of charged leptons and neutrinos is important to get clues o...
We explore some important implications of the KamLAND measurment on the lepton flavor mixing matrix ...
We introduce a simple flavor symmetry breaking scheme, in which charged lepton masses have a strong ...
Recently, many authors showed that if the solar and atmospheric neutrino data are both described by ...
We borrow the general idea of renormalization-group equations (RGEs) to understand how neutrino mass...
We propose a phenomenological model of lepton mixing and CP violation based on the flavor democracy ...
We provide a complete answer to the following question: what are the flavour groups and representat...
We show that the observed pattern for neutrino mixing arises naturally if neutrinos are composites o...