Phenomenological Study of Solar-Neutrino Induced Double Beta Decay of Mo100
arXiv:hep-ph/0204143 · doi:10.1023/A:1015344907452
Abstract
The detection of solar-neutrinos of different origin via induced beta beta process of Mo100 is investigated. The particular counting rates and energy distributions of emitted electrons are presented. A discussion in respect to solar-neutrino detector consisting of 10 tones of Mo100 is included. Both the cases of the standard solar model and neutrino oscillation scenarios are analyzed. Moreover, new beta^- beta^+ and beta^-/EC channels of the double-beta process are introduced and possibilities of their experimental observation are addressed.
arXiv comment8 pages, LaTeX, 2 postscript figures, Talk presented by P. Domin on the workshop MEDEX'01 (Prague, June, 2001), to appear in Czech. J. Phys. 52 (2002)
References in corpus (6)
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data
- Where do we stand with solar neutrino oscillations?
- How Uncertain Are Solar Neutrino Predictions?
- Phenomenology of Neutrino Oscillations
- Spectroscopy of Double-Beta and Inverse-Beta Decays from 100Mo for Neutrinos