Stellar (n,gamma) cross section of Ni-62
dc.contributor.author | Nassar, H. | en |
dc.contributor.author | Paul, M. | en |
dc.contributor.author | Ahmad, I. | en |
dc.contributor.author | Berkovits, D. | en |
dc.contributor.author | Bettan, M. | en |
dc.contributor.author | Collon, P. | en |
dc.contributor.author | Dababneh, S. | en |
dc.contributor.author | Ghelberg, S. | en |
dc.contributor.author | Greene, J. P. | en |
dc.contributor.author | Heger, A. | en |
dc.contributor.author | Heil, M. | en |
dc.contributor.author | Henderson, D. J. | en |
dc.contributor.author | Jiang, C. L. | en |
dc.contributor.author | Kappeler, F. | en |
dc.contributor.author | Koivisto, H. | en |
dc.contributor.author | O'Brien, S. | en |
dc.contributor.author | Pardo, R. C. | en |
dc.contributor.author | Patronis, N. | en |
dc.contributor.author | Pennington, T. | en |
dc.contributor.author | Plag, R. | en |
dc.contributor.author | Rehm, K. E. | en |
dc.contributor.author | Reifarth, R. | en |
dc.contributor.author | Scott, R. | en |
dc.contributor.author | Sinha, S. | en |
dc.contributor.author | Tang, X. | en |
dc.contributor.author | Vondrasek, R. | en |
dc.date.accessioned | 2015-11-24T18:34:57Z | |
dc.date.available | 2015-11-24T18:34:57Z | |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/17016 | |
dc.rights | Default Licence | - |
dc.subject | massive stars | en |
dc.subject | ion-source | en |
dc.subject | s-process | en |
dc.subject | capture | en |
dc.subject | nucleosynthesis | en |
dc.subject | separation | en |
dc.title | Stellar (n,gamma) cross section of Ni-62 | en |
heal.abstract | The Ni-62(n,gamma)Ni-63(t(1/2) = 100 +/- 2 yr) reaction plays an important role in the control of the flow path of the slow neutron-capture (s) nucleosynthesis process. We have measured for the first time the total cross section of this reaction for a quasi-Maxwellian (kT = 25 keV) neutron flux. The measurement was performed by fast-neutron activation, combined with accelerator mass spectrometry to detect directly the Ni-63 product nuclei. The experimental value of 28.4 +/- 2.8 mb, fairly consistent with a recent calculation, affects the calculated net yield of Ni-62 itself and the whole distribution of nuclei with 62 < A < 90 produced by the weak s process in massive stars. | en |
heal.access | campus | - |
heal.fullTextAvailability | TRUE | - |
heal.identifier.primary | Doi 10.1103/Physrevlett.94.092504 | - |
heal.identifier.secondary | <Go to ISI>://000227566000017 | - |
heal.identifier.secondary | http://prl.aps.org/abstract/PRL/v94/i9/e092504 | - |
heal.journalName | Phys Rev Lett | en |
heal.journalType | peer reviewed | - |
heal.language | en | - |
heal.publicationDate | 2005 | - |
heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
heal.type | journalArticle | - |
heal.type.el | Άρθρο Περιοδικού | el |
heal.type.en | Journal article | en |
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