Astrophysical S factor and reaction rate of 92,94Mo(p,) relevant to the p-process

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dc.contributor.authorHingu, Akashcs
dc.contributor.authorPrajapati, P Mcs
dc.contributor.authorMukherjee, Surjitcs
dc.contributor.authorPizzone, R.G.cs
dc.contributor.authorKatovský, Karelcs
dc.coverage.issue1cs
dc.coverage.volume275cs
dc.date.issued2023-06-01cs
dc.description.abstractLow energy proton capture cross sections on heavy isotopes are necessary for a better understanding of the astrophysical p-process. There are around 35 proton-rich stable isotopes between 74Se and 196Hg which are bypassed by the s-and r-processes. These are commonly referred as p-nuclei whose origin is still not completely understood. In the present study, proton capture reactions are studied on Mo isotopes at astrophysically relevant energies using nuclear modular code TALYS. Astrophysical S factor and reaction rates are also calculated inside a core-collapse supernova. The obtained results are compared with the literature data taken from EXFOR data library. In addition, the effect of different combinations of the nuclear input parameters entering the stellar reaction rate have been investigated.en
dc.formattextcs
dc.format.extent3cs
dc.format.mimetypeapplication/pdfcs
dc.identifier.citationEPJ Web of Conferences. 2023, vol. 275, issue 1, 3 p.en
dc.identifier.doi10.1051/epjconf/202327502006cs
dc.identifier.issn2100-014Xcs
dc.identifier.orcid0000-0001-9335-8199cs
dc.identifier.other184162cs
dc.identifier.researcheridK-2656-2016cs
dc.identifier.scopus6507230729cs
dc.identifier.urihttp://hdl.handle.net/11012/213629
dc.language.isoencs
dc.publisherEDP Sciencescs
dc.relation.ispartofEPJ Web of Conferencescs
dc.relation.urihttps://www.epj-conferences.org/articles/epjconf/abs/2023/01/epjconf_enas112023_02006/epjconf_enas112023_02006.htmlcs
dc.rightsCreative Commons Attribution 4.0 Internationalcs
dc.rights.accessopenAccesscs
dc.rights.sherpahttp://www.sherpa.ac.uk/romeo/issn/2100-014X/cs
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/cs
dc.subjectastrophysicsen
dc.subjects-prrocessen
dc.subjectMo-92en
dc.subjectMo-94en
dc.subjectTALYS codeen
dc.subjectcore-collapse supernovaen
dc.subjectEXFORen
dc.subjectstellar reaction ratesen
dc.titleAstrophysical S factor and reaction rate of 92,94Mo(p,) relevant to the p-processen
dc.type.driverarticleen
dc.type.statusPeer-revieweden
dc.type.versionpublishedVersionen
sync.item.dbidVAV-184162en
sync.item.dbtypeVAVen
sync.item.insts2025.02.03 15:40:13en
sync.item.modts2025.01.17 15:13:34en
thesis.grantorVysoké učení technické v Brně. Fakulta elektrotechniky a komunikačních technologií. Ústav elektroenergetikycs
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