Reply to ``Is $U_{e3}$ really related to the solar neutrino solutions?''
| dc.creator | Akhmedov, E. Kh. | |
| dc.creator | Branco, G. C. | |
| dc.creator | Rebelo, M. N. | |
| dc.date | 2000-07-04 | |
| dc.date.accessioned | 2026-07-07T03:41:57Z | |
| dc.date.available | 2026-07-07T03:41:57Z | |
| dc.description | In a recent paper [1] we showed that, assuming no fine tuning between certain elements of the neutrino mass matrix, one can link the element U_{e3} of the lepton mixing matrix to solar and atmospheric neutrino oscillation parameters. This result has been recently criticized by Haba and Suzuki [2]. In the present note we show that their criticism is not valid and just reflects their failure to understand the content of our paper. | |
| dc.description | LaTeX, 2 pages, no figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0007029 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0007029 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/39754 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Reply to ``Is $U_{e3}$ really related to the solar neutrino solutions?'' | |
| dc.type | text |