Gallium data variability and KamLAND
| dc.creator | Pulido, Joao | |
| dc.creator | Chauhan, Bhag | |
| dc.creator | Picariello, Marco | |
| dc.date | 2006-11-27 | |
| dc.date.accessioned | 2026-07-07T10:37:27Z | |
| dc.date.available | 2026-07-07T10:37:27Z | |
| dc.description | We present an alternative fit to the conventional solar+KamLAND one which takes into account the possible time dependence of the Ga data and relies on the partial conversion of active $\to$ sterile neutrinos via the magnetic moment/solar field interaction. We evaluate the prediction for the solar neutrino rates obtaining a fit of similar quality as the LMA one. We also evaluate the KamLAND antineutrino survival probability as a function of reactor distance and find a better agreement with data as compared to LMA. | |
| dc.description | 3 pages, 1 figure, presented at NOW2006, Sep.9-16, Otranto, Italy | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0611331 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0611331 | |
| dc.identifier | Nucl.Phys.Proc.Suppl.168:137-139,2007 | |
| dc.identifier | doi:10.1016/j.nuclphysbps.2007.02.069 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180387 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Gallium data variability and KamLAND | |
| dc.type | text |