Calculated solar-neutrino capture rate for a radiochemical 205 Tl-based solar-neutrino detector
arXiv:1912.05334 · doi:10.1103/PhysRevC.101.031302
Abstract
Radiochemical experiments for low-energy solar-neutrino detection have been making headlines by exploiting the isotopes \iso{Cl}{37} and \iso{Ga}{71}. Such a very low-threshold measurement of this type can also be performed using \iso{Tl}{205}, which has been considered for decades for this purpose. A unique feature of this detector nucleus is the integration is the solar-neutrino flux over millions of years owing to its long-living daughter \iso{Pb}{205}. In this study we have calculated for the first time the cross section for the charged-current solar-neutrino scattering off \iso{Tl}{205}. Taking into account the solar-model-predicted neutrino fluxes and the electron-neutrino survival probabilities, a solar-neutrino capture rate of 62.2 SNU is determined, a value significantly smaller than in previous estimates.
arXiv comment3 pages, 4 figures
References in corpus (5)
- New solar opacities, abundances, helioseismology, and neutrino fluxes
- Value of the axial-vector coupling strength in and decays: A review
- Simultaneous Precision Spectroscopy of , Be, and Solar Neutrinos with Borexino Phase-II
- The gallium anomaly revisited
- The charged current neutrino cross section for solar neutrinos, and background to \BBz\ experiments