dc.contributor.author | Ydrefors, Emanuel | |
dc.contributor.author | Almosly, Wafa | |
dc.contributor.author | Suhonen, Jouni | |
dc.date.accessioned | 2016-07-11T07:08:48Z | |
dc.date.available | 2016-07-11T07:08:48Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Ydrefors, 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.other | CONVID_24802608 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/50775 | |
dc.description.abstract | Supernova-(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.iso | eng | |
dc.publisher | Editura Academiei Romane; Academia Romana | |
dc.relation.ispartofseries | Romanian Journal of Physics | |
dc.relation.uri | http://www.nipne.ro/rjp/2015_60_5-6/0836_0846.pdf | |
dc.subject.other | neutrino-nucleus scattering | |
dc.subject.other | supernova neutrinos | |
dc.subject.other | neutral-current processes | |
dc.subject.other | charged-current processes | |
dc.subject.other | quasiparticle random-phase approximation | |
dc.subject.other | microscopic quasiparticle-phonon model | |
dc.title | Nuclear structure and neutrino-nucleus reactions at supernova energies | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201607063509 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2016-07-06T12:15:21Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.format.pagerange | 836-846 | |
dc.relation.issn | 1221-146X | |
dc.relation.numberinseries | 5-6 | |
dc.relation.volume | 60 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © the Authors, 2015. This is an open access article published by Editura Academiei Romane. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.type.okm | A1 | |