On solar neutrino fluxes in radiochemical experiments
| dc.creator | Ikhsanov, R. N. | |
| dc.creator | Gnedin, Yu. N. | |
| dc.creator | Miletsky, E. V. | |
| dc.date | 2005-12-08 | |
| dc.date.accessioned | 2026-07-07T06:54:12Z | |
| dc.date.available | 2026-07-07T06:54:12Z | |
| dc.description | We analyze fluctuations of the solar neutrino flux using data from the Homestake, GALLEX, GNO, SAGE and Super Kamiokande experiments. Spectral analysis and direct quantitative estimations show that the most stable variation of the solar neutrino flux is a quasi-five-year periodicity. The revised values of the mean solar neutrino flux are presented in Table 4. They were used to estimate the observed pp-flux of the solar electron neutrinos near the Earth. We consider two alternative explanations for the origin of a variable component of the solar neutrino deficit. | |
| dc.description | 18 pages, 4 figures, 5 tables, 27 references. The paper is extended version of the report presented on 9th International Pulkovo Conference on Solar Physics, Saint-Petersburg, Russia, July 4-9, 2005 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0512094 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0512094 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/105854 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | On solar neutrino fluxes in radiochemical experiments | |
| dc.type | text |