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dc.contributor.authorBorge, M. J. G.
dc.contributor.authorTolosa, A.
dc.contributor.authorCarmona, M.
dc.contributor.authorBerry, T.
dc.contributor.authorTengblad, O.
dc.contributor.authorNacher, E.
dc.contributor.authorParra, S.
dc.contributor.authorBriz, J. A.
dc.contributor.authorAguilera, P.
dc.contributor.authorAgramunt, J.
dc.contributor.authorAlgora, A.
dc.contributor.authorTain, J. L.
dc.contributor.authorSotty, C.
dc.contributor.authorRubio, B.
dc.contributor.authorRomero, J.
dc.contributor.authorPerea, A.
dc.contributor.authorOrrigo, S. E. J.
dc.contributor.authorOrce, N.
dc.contributor.authorMorales, A. I.
dc.contributor.authorMolina, F.
dc.contributor.authorMarroquin, I.
dc.contributor.authorLica, R.
dc.contributor.authorIllana, A.
dc.contributor.authorGuadilla, V.
dc.contributor.authorGelletly, W.
dc.contributor.authorGanioglu, E.
dc.contributor.authorFraile, L. M.
dc.date.accessioned2023-10-10T12:12:52Z
dc.date.available2023-10-10T12:12:52Z
dc.identifier.citationNacher E., Parra S., Briz J. A., Aguilera P., Agramunt J., Algora A., Berry T., Borge M. J. G., Carmona M., Fraile L. M., et al., "Beta decay along the N=Z line and its relevance in rp-process and X-Ray bursts", 10th Conference on Nuclear Physics in Astrophysics (NPA), Geneva, İsviçre, 5 - 09 Eylül 2022
dc.identifier.otherav_1c3fae86-3f7f-4ab7-abe3-2ba3c2a665f2
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/189971
dc.identifier.urihttps://avesis.istanbul.edu.tr/api/publication/1c3fae86-3f7f-4ab7-abe3-2ba3c2a665f2/file
dc.identifier.urihttps://doi.org/10.1051/epjconf/202327912004
dc.description.abstractNucleosynthesis in Type I X-ray bursts (XRB) proceeds eventually through the rp-process near the proton drip-line. Several N=Z nuclei act as waiting points in the reaction network chain. Astrophysical calculations of XRB light curves depend upon the theoretical modelling of the beta decays of interest, with the N=Z waiting points Ge-64, Se-68, Kr-72, Sr-76, and their second-neighbours N=Z+2 being key nuclei in this context. We have carried out different experimental campaigns at ISOLDE (CERN) to determine the B(GT) distributions, in the decay of several N=Z, N=Z+2 and their daughters, of particular relevance in rp-process calculations. To this aim the Total Absorption Spectroscopy technique is applied. Here we present results on the beta decay of Ga-64 and the status of the analysis of Ge-64. Our results provide benchmarks for testing and constraining models under terrestrial conditions that can be used later for predictions in stellar environments.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectFİZİK, NÜKLEER
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik Bilimleri
dc.subjectUzay ve Gezegen Bilimi
dc.subjectGenel Fizik ve Astronomi
dc.subjectFizik ve Astronomi (çeşitli)
dc.subjectNükleer ve Yüksek Enerji Fiziği
dc.subjectTemel Bilimler
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectAstronomi ve Astrofizik
dc.subjectFİZİK, PARÇACIKLAR VE ALANLAR
dc.titleBeta decay along the N=Z line and its relevance in rp-process and X-Ray bursts
dc.typeBildiri
dc.contributor.departmentCSIC Univ Valencia , ,
dc.contributor.firstauthorID4313936


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