Skip navigation

Zastosuj identyfikator do podlinkowania lub zacytowania tej pozycji: http://hdl.handle.net/20.500.12128/6962
Pełny rekord metadanych
DC poleWartośćJęzyk
dc.contributor.authorCzakon, Michał-
dc.contributor.authorStudnik, J.-
dc.contributor.authorZrałek, Marek-
dc.contributor.authorGluza, Janusz-
dc.date.accessioned2018-11-06T12:06:51Z-
dc.date.available2018-11-06T12:06:51Z-
dc.date.issued2000-
dc.identifier.citationActa Physica Polonica. B, 2000, no. no. 6, s. 1365-1387pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/6962-
dc.description.abstractThe neutrinoless double beta decay as well as any other laboratory experiment has not been able to answer the question of the neutrino’s nature. Hints on the answer are available when neutrino oscillations and (/3/3)qv are considered simultaneously. In this case phenomenologically interesting neutrino mass schemes can lead to non-vanishing and large values of (mv). As a consequence, some schemes with Majorana neutrinos can be ruled out even now. If we assume that in addition neutrinos contribute to Hot Dark Matter then the window for Majorana neutrinos is even more restricted, e.g. GENIUS experiment will be sensitive to scenarios with three Majorana neutrinos[…]pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectoscylacje neutrinpl_PL
dc.subjectfizyka jądrowapl_PL
dc.titleGENIUS project, neutrino oscillations and cosmology : neutrinos reveal their nature?.pl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.relation.journalActa Physica Polonica. Bpl_PL
Pojawia się w kolekcji:Artykuły (WNŚiT)

Pliki tej pozycji:
Plik Opis RozmiarFormat 
Czakon_Genius_project_neutrino.pdf606,3 kBAdobe PDFPrzejrzyj / Otwórz
Pokaż prosty rekord


Uznanie Autorstwa 3.0 Polska Creative Commons Creative Commons