dc.contributor.author | WELKER, A. | |
dc.contributor.author | KISLER, D. | |
dc.contributor.author | LITVINOV, Yu. A. | |
dc.contributor.author | Lunney, D. | |
dc.contributor.author | Manea, V. | |
dc.contributor.author | Neidherr, D. | |
dc.contributor.author | Rosenbusch, M. | |
dc.contributor.author | Schweikhard, L. | |
dc.contributor.author | Wienholtz, F. | |
dc.contributor.author | Wolf, R. N. | |
dc.contributor.author | Zuber, K. | |
dc.contributor.author | Cocolios, T. E. | |
dc.contributor.author | George, S. | |
dc.contributor.author | Goriely, S. | |
dc.contributor.author | Herfurth, F. | |
dc.contributor.author | JANKA, H. -T. | |
dc.contributor.author | JUST, O. | |
dc.contributor.author | Kowalska, M. | |
dc.contributor.author | Kreim, S. | |
dc.contributor.author | Atanasov, D. | |
dc.contributor.author | Ascher, P. | |
dc.contributor.author | Blaum, K. | |
dc.contributor.author | Cakirli, Rabia Burcu | |
dc.date.accessioned | 2021-03-05T19:30:02Z | |
dc.date.available | 2021-03-05T19:30:02Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Atanasov D., Ascher P., Blaum K., Cakirli R. B. , Cocolios T. E. , George S., Goriely S., Herfurth F., JANKA H. -. , JUST O., et al., "Precision Mass Measurements of Cd129-131 and Their Impact on Stellar Nucleosynthesis via the Rapid Neutron Capture Process", PHYSICAL REVIEW LETTERS, cilt.115, 2015 | |
dc.identifier.issn | 0031-9007 | |
dc.identifier.other | av_cf90dc6e-483c-439f-96ae-1e00bd923a72 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/137247 | |
dc.identifier.uri | https://doi.org/10.1103/physrevlett.115.232501 | |
dc.description.abstract | Masses adjacent to the classical waiting-point nuclide Cd-130 have been measured by using the Penningtrap spectrometer ISOLTRAP at ISOLDE/CERN. We find a significant deviation of over 400 keV from earlier values evaluated by using nuclear beta-decay data. The new measurements show the reduction of the N = 82 shell gap below the doubly magic Sn-132. The nucleosynthesis associated with the ejected wind from type-II supernovae as well as from compact object binary mergers is studied, by using state-of-the-art hydrodynamic simulations. We find a consistent and direct impact of the newly measured masses on the calculated abundances in the A = 128-132 region and a reduction of the uncertainties from the precision mass input data. | |
dc.language.iso | eng | |
dc.subject | Disiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları | |
dc.subject | FİZİK, MULTİDİSİPLİNER | |
dc.subject | Fizik | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Temel Bilimler | |
dc.title | Precision Mass Measurements of Cd129-131 and Their Impact on Stellar Nucleosynthesis via the Rapid Neutron Capture Process | |
dc.type | Makale | |
dc.relation.journal | PHYSICAL REVIEW LETTERS | |
dc.contributor.department | , , | |
dc.identifier.volume | 115 | |
dc.identifier.issue | 23 | |
dc.contributor.firstauthorID | 79888 | |