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dc.contributor.authorAlmosly, Wafa
dc.contributor.authorCarlsson, B. G.
dc.contributor.authorSuhonen, Jouni
dc.contributor.authorYdrefors, E.
dc.date.accessioned2019-05-29T06:08:06Z
dc.date.available2019-05-29T06:08:06Z
dc.date.issued2019fi
dc.identifier.citationAlmosly, W., Carlsson, B. G., Suhonen, J., & Ydrefors, E. (2019). Neutral-current supernova-neutrino cross sections for 204,206,208Pb calculated by Skyrme quasiparticle random-phase approximation. <em>Physical Review C</em>, 99 (5), 055801. <a href="https://doi.org/10.1103/PhysRevC.99.055801">doi:10.1103/PhysRevC.99.055801</a>fi
dc.identifier.otherTUTKAID_81341
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/64260
dc.description.abstractThe present work constitutes a detailed study of neutral-current (NC) supernova-neutrino scattering off the stable even-even lead isotopes 204,206,208Pb. This is a continuation of our previous work [Almosly et al., Phys. Rev. C. 94, 044614 (2016)] where we investigated charged-current processes on the same nuclei. As in the previous work, we have adopted the quasiparticle random-phase approximation (QRPA) as the theory framework and use three different Skyrme interactions to build the involved nuclear wave functions. We test the Skyrme forces by computing the location of the lowest-order isovector spin-multipole giant resonances and comparing with earlier calculations. We have computed the NC cross sections for (anti)neutrino energies up to 100 MeV and estimated the nuclear responses to supernova (anti)neutrinos by folding the obtained cross sections by suitably parametrized Fermi-Dirac distributions of energies of the incoming (anti)neutrinos. We compare our results with results of earlier studies in the case of 208Pb, which is the only lead isotope where earlier calculations are available.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.othercollective levelsfi
dc.subject.othernuclear forcesfi
dc.subject.othernucleus-neutrino interactionsfi
dc.titleNeutral-current supernova-neutrino cross sections for 204,206,208Pb calculated by Skyrme quasiparticle random-phase approximationfi
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201905062408
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2019-05-06T09:15:37Z
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries5
dc.relation.volume99
dc.type.versionpublishedVersion
dc.rights.copyright©2019 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.format.contentfulltext
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.99.055801


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