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dc.contributor.authorYdrefors, Emanuel
dc.contributor.authorAlmosly, Wafa
dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2016-07-11T07:08:48Z
dc.date.available2016-07-11T07:08:48Z
dc.date.issued2015
dc.identifier.citationYdrefors, E., Almosly, W., & Suhonen, J. (2015). Nuclear structure and neutrino-nucleus reactions at supernova energies. <i>Romanian Journal of Physics</i>, <i>60</i>(5-6), 836-846. <a href="http://www.nipne.ro/rjp/2015_60_5-6/0836_0846.pdf" target="_blank">http://www.nipne.ro/rjp/2015_60_5-6/0836_0846.pdf</a>
dc.identifier.otherCONVID_24802608
dc.identifier.otherTUTKAID_66657
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/50775
dc.description.abstractSupernova-(anti-)neutrino–nucleus scattering is discussed with reference to neutral-current (NC) and charged-current (CC) processes in heavy stable nuclei. The Donnelly-Walecka method with the associated multipole expansion of the nucleonic current has been adopted as the basic framework in deriving the neutrino-nucleus scattering cross sections. The needed nuclear wave functions are computed by using the quasiparticle random-phase approximation (QRPA) for the even-even target nuclei in the NC processes and the proton-neutron QRPA (pnQRPA) has been used to compute the CC processes for the mentioned nuclei. The wave functions of the stable odd-mass target nuclei have been obtained by the use of the QRPA-based microscopic quasiparticle-phonon model (MQPM), applied to both NC and CC processes. The obtained cross sections are folded by the energy distributions of the various (anti-)neutrino flavors in order to access detection rates in Earth-based neutrino telescopes. The stable molybdenum (Mo) nuclei serve as examples of application of the formalism, with a subsequent analysis of the results.
dc.language.isoeng
dc.publisherEditura Academiei Romane; Academia Romana
dc.relation.ispartofseriesRomanian Journal of Physics
dc.relation.urihttp://www.nipne.ro/rjp/2015_60_5-6/0836_0846.pdf
dc.subject.otherneutrino-nucleus scattering
dc.subject.othersupernova neutrinos
dc.subject.otherneutral-current processes
dc.subject.othercharged-current processes
dc.subject.otherquasiparticle random-phase approximation
dc.subject.othermicroscopic quasiparticle-phonon model
dc.titleNuclear structure and neutrino-nucleus reactions at supernova energies
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201607063509
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-07-06T12:15:21Z
dc.type.coarjournal article
dc.description.reviewstatuspeerReviewed
dc.format.pagerange836-846
dc.relation.issn1221-146X
dc.relation.numberinseries5-6
dc.relation.volume60
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2015. This is an open access article published by Editura Academiei Romane.
dc.rights.accesslevelopenAccessfi


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