Solar Neutrino Background in Neutrinoless double beta-decay searching for experiments
| dc.creator | Klimenko, Alexander A. | |
| dc.date | 2004-07-14 | |
| dc.date.accessioned | 2026-07-07T03:52:52Z | |
| dc.date.available | 2026-07-07T03:52:52Z | |
| dc.description | Background of germanium and xenon detectors due to the elastic scattering of $^{8}B$ solar neutrinos on electrons have been calculated. The background is 4.6 \times $10^{-4}$ counts/(keV$\cdot t\cdot$y) that defines the sensitivity of double beta-decay experiments at a level $T^{0νββ}_{1/2} \approx 4\times$10^{27}$ {yr} and it corresponds to effective majorana mass $ \mid < m_{ν_e}>\mid \approx 23.5$ meV. This limit after a half of one year of measurements for 10 tons natural Xe detector will be obtained. | |
| dc.description | 3 pages, 2 figures Talk given at LIV International Meeting on Nuclear Spectroscopy and Nuclear Structure "NUCLEUS-2004" June 22-25, 2004, Belgorod, Russia Section #6 Fundamental Interactions in Nuclear Physics Formula correction | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0407156 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0407156 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/43627 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Solar Neutrino Background in Neutrinoless double beta-decay searching for experiments | |
| dc.type | text |