A Lithium Experiment in the Program of Solar Neutrino Research
| dc.creator | Kopylov, A. | |
| dc.creator | Orekhov, I. | |
| dc.creator | Petukhov, V. | |
| dc.creator | Solomatin, A. | |
| dc.date | 2006-01-12 | |
| dc.date.accessioned | 2026-07-07T10:29:50Z | |
| dc.date.available | 2026-07-07T10:29:50Z | |
| dc.description | The experiments sensitive to pp-neutrinos from the Sun are very perspective for the precise measurement of a mixing angle $θ_{12}$. A $ν$e$^{-}$ scattering experiment (Xmass) and/or a charged-current experiment (the indium detector) can measure the flux of electron pp-neutrinos. One can find the total flux of pp-neutrinos from a luminosity constraint after the contribution of $^7$Be and CNO neutrinos to the total luminosity of the Sun are measured. The radiochemical experiment utilizing a lithium target has the high sensitivity to the CNO neutrinos, thus, it has a good promise for the precise measurement of a mixing angle and for the test of a current theory of the evolution of the stars. | |
| dc.description | 6 pages, 2 figures, 1 table, A report made by A.Kopylov at International Conference NANP-2005, June 2005, Dubna, Russia | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0601091 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0601091 | |
| dc.identifier | Phys.Atom.Nucl.69:1829-1832,2006 | |
| dc.identifier | doi:10.1134/S1063778806110044 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177945 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A Lithium Experiment in the Program of Solar Neutrino Research | |
| dc.type | text |