dc.contributor.author | Borge, M. J. G. | |
dc.contributor.author | Tolosa, A. | |
dc.contributor.author | Carmona, M. | |
dc.contributor.author | Berry, T. | |
dc.contributor.author | Tengblad, O. | |
dc.contributor.author | Nacher, E. | |
dc.contributor.author | Parra, S. | |
dc.contributor.author | Briz, J. A. | |
dc.contributor.author | Aguilera, P. | |
dc.contributor.author | Agramunt, J. | |
dc.contributor.author | Algora, A. | |
dc.contributor.author | Tain, J. L. | |
dc.contributor.author | Sotty, C. | |
dc.contributor.author | Rubio, B. | |
dc.contributor.author | Romero, J. | |
dc.contributor.author | Perea, A. | |
dc.contributor.author | Orrigo, S. E. J. | |
dc.contributor.author | Orce, N. | |
dc.contributor.author | Morales, A. I. | |
dc.contributor.author | Molina, F. | |
dc.contributor.author | Marroquin, I. | |
dc.contributor.author | Lica, R. | |
dc.contributor.author | Illana, A. | |
dc.contributor.author | Guadilla, V. | |
dc.contributor.author | Gelletly, W. | |
dc.contributor.author | Ganioglu, E. | |
dc.contributor.author | Fraile, L. M. | |
dc.date.accessioned | 2023-10-10T12:12:52Z | |
dc.date.available | 2023-10-10T12:12:52Z | |
dc.identifier.citation | Nacher 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.other | av_1c3fae86-3f7f-4ab7-abe3-2ba3c2a665f2 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/189971 | |
dc.identifier.uri | https://avesis.istanbul.edu.tr/api/publication/1c3fae86-3f7f-4ab7-abe3-2ba3c2a665f2/file | |
dc.identifier.uri | https://doi.org/10.1051/epjconf/202327912004 | |
dc.description.abstract | Nucleosynthesis 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.iso | eng | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Fizik | |
dc.subject | FİZİK, NÜKLEER | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.subject | Uzay bilimi | |
dc.subject | Fizik Bilimleri | |
dc.subject | Uzay ve Gezegen Bilimi | |
dc.subject | Genel Fizik ve Astronomi | |
dc.subject | Fizik ve Astronomi (çeşitli) | |
dc.subject | Nükleer ve Yüksek Enerji Fiziği | |
dc.subject | Temel Bilimler | |
dc.subject | Temel Parçacıklar ve Alanlar | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | FİZİK, PARÇACIKLAR VE ALANLAR | |
dc.title | Beta decay along the N=Z line and its relevance in rp-process and X-Ray bursts | |
dc.type | Bildiri | |
dc.contributor.department | CSIC Univ Valencia , , | |
dc.contributor.firstauthorID | 4313936 | |