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dc.contributor.authorTsakstara, V.en
dc.contributor.authorKosmas, T. S.en
dc.contributor.authorDivari, P. C.en
dc.contributor.authorSinatkas, J.en
dc.date.accessioned2015-11-24T18:34:32Z-
dc.date.available2015-11-24T18:34:32Z-
dc.identifier.issn0146-6410-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16958-
dc.rightsDefault Licence-
dc.subjectneutrino nucleus cross sectionsen
dc.subjectsupernova neutrino detectionen
dc.subjectnuclear detector responseen
dc.subjectquasi-particle random phase approximationen
dc.titleSupernova neutrino detection by terrestrial nuclear detectorsen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDOI 10.1016/j.ppnp.2009.12.061-
heal.identifier.secondary<Go to ISI>://000283519100062-
heal.identifier.secondaryhttp://ac.els-cdn.com/S0146641009001392/1-s2.0-S0146641009001392-main.pdf?_tid=b1bb359de4a2efdae0aa3db9fc435ebd&acdnat=1334228774_0f8be03a994aba21ef5f1d1ebeaf1e25-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2010-
heal.abstractWe present and discuss differential cross sections for the (128.13)Te isotopes, contents of the COBRA double beta decay detector. The response of these isotopes to energy spectra of supernova neutrinos is explored by convoluting the original results, calculated in the context of the quasi-particle random phase approximation (QRPA) using realistic two-body forces, with a two-parameter Fermi-Dirac (FD) and a Power-Law (PL) neutrino energy distributions. (C) 2009 Elsevier B.V. All rights reserved.en
heal.journalNameProgress in Particle and Nuclear Physicsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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