DC pole | Wartość | Język |
dc.contributor.author | Joniec, Agnieszka | - |
dc.contributor.author | Zrałek, Marek | - |
dc.date.accessioned | 2018-11-29T12:22:08Z | - |
dc.date.available | 2018-11-29T12:22:08Z | - |
dc.date.issued | 2004 | - |
dc.identifier.citation | Acta Physica Polonica. B, 2004, no. 2, s. 639-646 | pl_PL |
dc.identifier.issn | 0587-4254 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/7287 | - |
dc.description.abstract | Presently the best terrestrial limit on light neutrino masses (m<2.2 eV)
are given by the tritium beta decay experiments. Not maximal mixing
of solar neutrinos following from the SNO and KamLAND together with
neutrinoless double beta decay (( )0 ) data open the chance for better
determination of the lightest of Majorana neutrino mass. We combine all
available fits for the solar neutrino parameters and collect all Nuclear Matrix
Elements (NME) calculations for the 76Ge, nucleus for which presently
the most stringent limit on the ( )0 decay half-life time exist. We have
shown that for some NME smaller bound on (m )min can be found. Unfortunately
one order of magnitude discrepancies in NME calculations do
not allow to give the final answer. | pl_PL |
dc.language.iso | en | pl_PL |
dc.rights | Uznanie autorstwa 3.0 Polska | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/pl/ | * |
dc.subject | Majorana neutrinos | pl_PL |
dc.subject | neutrino | pl_PL |
dc.title | Bound on the mass of Majorana neutrinos after SNO and KamLAND | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
dc.relation.journal | Acta Physica Polonica. B | pl_PL |
Pojawia się w kolekcji: | Artykuły (WNŚiT)
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