The polarized electron target as a new solar-neutrino detector
arXiv:astro-ph/0502522 · doi:10.1016/j.nuclphysb.2005.11.020
Abstract
In this paper, we analyze the scattering of solar neutrinos on the polarized electron target, and predict how the effect of parity violation in weak interactions may help to distinguish neutrino signal from detector background. We indicate that the knowledge of the Sun motion across the sky is sufficient to predict the day/night asymmetry in the scattering on the polarized electron target. To make this detection feasible, the polarized electron target for solar neutrinos needs to be build from magnetic materials, e.g. from ferromagnetic iron foils, paramagnetic scintillator crystals or scintillating ferrofluids.
arXiv comment3 pages, 2 eps figures, revtex
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- Quantum flavor oscillations extended to the Dirac theory
- Theoretical correlation between possible evidences of neutrino chiral oscillations and polarization measurements
- Neutrino elastic scattering on polarized electrons as a tool for probing the neutrino nature
- On possibility of time reversal symmetry violation in neutrino elastic scattering on polarized electron target
- CP violation in scattering of neutrinos on polarized proton target
- Recoil electron polarization-dependent T-odd correlations in neutrino elastic scattering on polarized electron target