(96)Zr(n,gamma) measurement at the n_TOF facility at CERN
dc.contributor.author | Tagliente, G. | en |
dc.contributor.author | Milazzo, P. M. | en |
dc.contributor.author | Fujii, K. | en |
dc.contributor.author | Abbondanno, U. | en |
dc.contributor.author | Aerts, G. | en |
dc.contributor.author | Alvarez, H. | en |
dc.contributor.author | Alvarez-Velarde, F. | en |
dc.contributor.author | Andriamonje, S. | en |
dc.contributor.author | Andrzejewski, J. | en |
dc.contributor.author | Audouin, L. | en |
dc.contributor.author | Badurek, G. | en |
dc.contributor.author | Baumann, P. | en |
dc.contributor.author | Becvar, F. | en |
dc.contributor.author | Belloni, F. | en |
dc.contributor.author | Berthoumieux, E. | en |
dc.contributor.author | Calvino, F. | en |
dc.contributor.author | Calviani, M. | en |
dc.contributor.author | Cano-Ott, D. | en |
dc.contributor.author | Capote, R. | en |
dc.contributor.author | Carrapico, C. | en |
dc.contributor.author | Cennini, P. | en |
dc.contributor.author | Chepel, V. | en |
dc.contributor.author | Chiaveri, E. | en |
dc.contributor.author | Colonna, N. | en |
dc.contributor.author | Cortes, G. | en |
dc.contributor.author | Couture, A. | en |
dc.contributor.author | Dahlfors, M. | en |
dc.contributor.author | David, S. | en |
dc.contributor.author | Dillmann, I. | en |
dc.contributor.author | Domingo-Pardo, C. | en |
dc.contributor.author | Dridi, W. | en |
dc.contributor.author | Duran, I. | en |
dc.contributor.author | Eleftheriadis, C. | en |
dc.contributor.author | Embid-Segura, M. | en |
dc.contributor.author | Ferrari, A. | en |
dc.contributor.author | Ferreira-Marques, R. | en |
dc.contributor.author | Furman, W. | en |
dc.contributor.author | Goncalves, I. | en |
dc.contributor.author | Gonzalez-Romero, E. | en |
dc.contributor.author | Gramegna, F. | en |
dc.contributor.author | Guerrero, C. | en |
dc.contributor.author | Gunsing, F. | en |
dc.contributor.author | Haas, B. | en |
dc.contributor.author | Haight, R. | en |
dc.contributor.author | Heil, M. | en |
dc.contributor.author | Herrera-Martinez, A. | en |
dc.contributor.author | Jericha, E. | en |
dc.contributor.author | Kappeler, F. | en |
dc.contributor.author | Kadi, Y. | en |
dc.contributor.author | Karadimos, D. | en |
dc.contributor.author | Karamanis, D. | en |
dc.contributor.author | Kerveno, M. | en |
dc.contributor.author | Kossionides, E. | en |
dc.contributor.author | Krticka, M. | en |
dc.contributor.author | Lamboudis, C. | en |
dc.contributor.author | Leeb, H. | en |
dc.contributor.author | Lindote, A. | en |
dc.contributor.author | Lopes, I. | en |
dc.contributor.author | Lukic, S. | en |
dc.contributor.author | Marganiec, J. | en |
dc.contributor.author | Marrone, S. | en |
dc.contributor.author | Martinez, T. | en |
dc.contributor.author | Massimi, C. | en |
dc.contributor.author | Mastinu, P. | en |
dc.contributor.author | Mengoni, A. | en |
dc.contributor.author | Moreau, C. | en |
dc.contributor.author | Mosconi, M. | en |
dc.contributor.author | Neves, F. | en |
dc.contributor.author | Oberhummer, H. | en |
dc.contributor.author | O'Brien, S. | en |
dc.contributor.author | Pancin, J. | en |
dc.contributor.author | Papachristodoulou, C. | en |
dc.contributor.author | Papadopoulos, C. | en |
dc.contributor.author | Paradela, C. | en |
dc.contributor.author | Patronis, N. | en |
dc.contributor.author | Pavlik, A. | en |
dc.contributor.author | Pavlopoulos, P. | en |
dc.contributor.author | Perrot, L. | en |
dc.contributor.author | Pigni, M. T. | en |
dc.contributor.author | Plag, R. | en |
dc.contributor.author | Plompen, A. | en |
dc.contributor.author | Plukis, A. | en |
dc.contributor.author | Poch, A. | en |
dc.contributor.author | Praena, J. | en |
dc.contributor.author | Pretel, C. | en |
dc.contributor.author | Quesada, J. | en |
dc.contributor.author | Reifarth, R. | en |
dc.contributor.author | Rosetti, M. | en |
dc.contributor.author | Rubbia, C. | en |
dc.contributor.author | Rudolf, G. | en |
dc.contributor.author | Rullhusen, P. | en |
dc.contributor.author | Salgado, J. | en |
dc.contributor.author | Santos, C. | en |
dc.contributor.author | Sarchiapone, L. | en |
dc.contributor.author | Savvidis, I. | en |
dc.contributor.author | Stephan, C. | en |
dc.contributor.author | Tain, J. L. | en |
dc.contributor.author | Tassan-Got, L. | en |
dc.contributor.author | Tavora, L. | en |
dc.contributor.author | Terlizzi, R. | en |
dc.contributor.author | Vannini, G. | en |
dc.contributor.author | Vaz, P. | en |
dc.contributor.author | Ventura, A. | en |
dc.contributor.author | Villamarin, D. | en |
dc.contributor.author | Vincente, M. C. | en |
dc.contributor.author | Vlachoudis, V. | en |
dc.contributor.author | Vlastou, R. | en |
dc.contributor.author | Voss, F. | en |
dc.contributor.author | Walter, S. | en |
dc.contributor.author | Wiescher, M. | en |
dc.contributor.author | Wisshak, K. | en |
dc.contributor.author | N TOF Collaboration | en |
dc.date.accessioned | 2015-11-24T18:33:50Z | |
dc.date.available | 2015-11-24T18:33:50Z | |
dc.identifier.issn | 0556-2813 | - |
dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16819 | |
dc.rights | Default Licence | - |
dc.subject | giant branch stars | en |
dc.subject | capture cross-sections | en |
dc.subject | s-process nucleosynthesis | en |
dc.subject | neutron-capture | en |
dc.subject | massive stars | en |
dc.subject | primitive meteorites | en |
dc.subject | statistical-model | en |
dc.subject | nuclear-science | en |
dc.subject | silicon-carbide | en |
dc.subject | elements | en |
dc.title | (96)Zr(n,gamma) measurement at the n_TOF facility at CERN | en |
heal.abstract | The (n,gamma) cross section of (96)Zr has been investigated at the CERN n_TOF spallation neutron source. High-resolution time-of-flight measurements using an enriched ZrO(2) sample allowed us to analyze 15 resonances below 40 keV with improved accuracy. On average, the capture widths were found to be 25% smaller than reported in earlier experiments. If complemented with the contribution by direct radiative capture, the derived Maxwellian averaged cross sections are consistent with activation data at kT = 25 keV. The present results confirm the astrophysical implications for the s-process branching at (95)Zr. | en |
heal.access | campus | - |
heal.fullTextAvailability | TRUE | - |
heal.identifier.secondary | <Go to ISI>://000297121100005 | - |
heal.identifier.secondary | http://prc.aps.org/abstract/PRC/v84/i5/e055802 | - |
heal.journalName | Physical Review C | en |
heal.journalType | peer reviewed | - |
heal.language | en | - |
heal.publicationDate | 2011 | - |
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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