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Detecting dark energy in long baseline neutrino oscillations
dark energy neutrino oscillation
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2009/8/14
In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type o...
On some properties of the neutrino in the early universe
neutrino early universe
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2010/4/8
Properties of the neutrino in the early universe have been investigated incorporating a small inhomogeneity in the mass density of the early universe. Dependence on this factor is found in studying me...
Combined Analysis of Solar Neutrino Data within The RSFP Framework Together with New KamLAND Data
Neutrino magnetic moment RSFP
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2010/4/8
A combined analysis of solar neutrino data together with the new KamLAND data is presented in the RSFP framework. It is investigated how the allowed regions are effected from the new KamLAND data at d...
Study of second-class currents effects on polarization characteristics in quasi-elastic neutrino (anti-neutrino) scattering by nuclei
Second-class currents nuclei polarization neutrino scattering spin asymmetry and en correlation
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2010/4/8
The differential cross section of quasi-elastic neutrino scattering by nuclei is computed. The numerical analysis of energy dependence of the spin asymmetry, the angular electron-neutrino (en) correla...
Neutrino Physics: the Roadmap for Precision Physics
Neutrinos Neutrino oscillation
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2010/10/13
In the last years, we experienced a complete change of the view of weak interaction physics. Robust results from many experiments as Super-Kamiokande, KamLAND, SNO, K2K, show us that the neutrinos hav...
KamLAND Data and the Solution to the Solar Neutrino Problem
KamLAND Data the Solution the Solar Neutrino Problem
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2010/10/26
KamLAND Data and the Solution to the Solar Neutrino Problem.
Influence of the Solar and Density Perturbations on the Neutrino Parameters
the Solar and Density Perturbations the Neutrino Parameters
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2010/10/27
There are reasons to believe that the solar matter density fluctuates around an equilibrium profile. One of these reasons is a resonance between the Alfv´en waves and the g-modes inside the Sun ...
Field and Polarization Effects Arising in Neutrino-Lepton Processes in a Magnetic Field
Polarization Effects Magnetic Field Neutrino-Lepton Processes
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2010/4/15
We discuss the effects arising in the neutrino-lepton processes (nm+e- \rightarrow ne+m- and \overline{n}e+e-\rightarrow\overline{n}m+m-) in a constant uniform magnetic field in the framework of the W...