301. Experimental neutron capture data of 58Ni from the CERN n-TOF facility
- Author
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M. B. Gómez-Hornillos, Christoph Langer, M. Mirea, Petar Žugec, A. K. Saxena, J. Billowes, F. Cerutti, Arnaud Ferrari, H. Leeb, A. J. M. Plompen, G. Vannini, P. Vaz, J. Perkowski, G. Tagliente, Alberto Ventura, Rene Reifarth, V. Bécares, M. Krtička, F. Calviño, Stefan Schmidt, D. Cano-Ott, Alberto Mengoni, S. Heinitz, Vittorio Boccone, M. Diakaki, C. Paradela, Mario Weigand, J. M. Quesada, L. Tassan-Got, E. Jericha, L. Audouin, G. Cortes, Javier Praena, S. Lo Meo, V. Variale, D. Tarrío, M. Kokkoris, J. L. Tain, Dorothea Schumann, C. Weiß, T. Martinez, Rugard Dressler, Jeri Kroll, Roberto Versaci, A. Tsinganis, G. Giubrone, Carlos Guerrero, Nicola Colonna, S. Altstadt, A. Pavlik, R. Sarmento, L.S. Leong, Vasilis Vlachoudis, C. Rubbia, F. Mingrone, J. Andrzejewski, C. Domingo-Pardo, A. Riegov, T. J. Wright, A. Manousos, J. Marganiec, I. F. Gonçalves, F. Bečvář, Roberto Losito, E. Mendoza, P. M. Milazzo, Peter Schillebeeckx, N. Dzysiuk, K. Fraval, F. Gunsing, C. Lederer, R. Vlastou, Fabio Belloni, E. Chiaveri, E. Berthoumieux, P. F. Mastinu, Cristian Massimi, Marco Pignatari, Damir Bosnar, Y. Kadi, S. Valenta, Marco Calviani, F. Käppeler, N. Kivel, P. Gurusamy, M. Meaze, M. J. Vermeulen, W. Mondalaers, M. Mastromarco, C. Carrapiço, Anton Wallner, I. Duran, D. G. Jenkins, M. A. Cortés-Giraldo, P. E. Koehler, T. Ware, E. Griesmayer, A. R. García, M. Brugger, Srinivasan Ganesan, Mario Barbagallo, M. P. W. Chin, F. Roman, C. Eleftheriadis, Thomas Rauscher, D. Karadimos, E. González-Romero, Žugec, P., Barbagallo, M., Colonna, N., Bosnar, D., Altstadt, S., Andrzejewski, J., Audouin, L., Bécares, V., Bečvář, F., Belloni, F., Berthoumieux, E., Billowes, J., Boccone, V., Brugger, M., Calviani, M., Calviño, F., Cano-Ott, D., Carrapiço, C., Cerutti, F., Chiaveri, E., Chin, M., Cortés, G., Cortés-Giraldo, M.A., Diakaki, M., Domingo-Pardo, C., Dressler, R., Duran, I., Dzysiuk, N., Eleftheriadis, C., Ferrari, A., Fraval, K., Ganesan, S., García, A.R., Giubrone, G., Gómez-Hornillos, M.B., Gonçalves, I.F., González-Romero, E., Griesmayer, E., Guerrero, C., Gunsing, F., Gurusamy, P., Heinitz, S., Jenkins, D.G., Jericha, E., Kadi, Y., Käppeler, F., Karadimos, D., Kivel, N., Koehler, P., Kokkoris, M., Krtička, M., Kroll, J., Langer, C., Lederer, C., Leeb, H., Leong, L.S., Lo Meo, S., Losito, R., Manousos, A., Marganiec, J., Martínez, T., Massimi, C., Mastinu, P.F., Mastromarco, M., Meaze, M., Mendoza, E., Mengoni, A., Milazzo, P.M., Mingrone, F., Mirea, M., Mondalaers, W., Paradela, C., Pavlik, A., Perkowski, J., Pignatari, M., Plompen, A., Praena, J., Quesada, J.M., Rauscher, T., Reifarth, R., Riegov, A., Roman, F., Rubbia, C., Sarmento, R., Saxena, A., Schillebeeckx, P., Schmidt, S., Schumann, D., Tagliente, G., Tain, J.L., Tarrío, D., Tassan-Got, L., Tsinganis, A., Valenta, S., Vannini, G., Variale, V., Vaz, P., Ventura, A., Versaci, R., Vermeulen, M.J., Vlachoudis, V., Vlastou, R., Wallner, A., Ware, T., Weigand, M., Weiß, C., Wright, T., Universitat Politècnica de Catalunya. Departament de Física, and Universitat Politècnica de Catalunya. ANT - Advanced Nuclear Technologies Research Group
- Subjects
Nuclear reaction ,nTOF ,Physics::Instrumentation and Detectors ,QC1-999 ,Astrophysics::High Energy Astrophysical Phenomena ,Neutron ,Nuclear physics ,Physics and Astronomy (all) ,CERN ,Neutron cross section ,Nuclear Experiment ,Energies::Energia nuclear [Àrees temàtiques de la UPC] ,Neutrons ,Physics ,Large Hadron Collider ,Física [Àrees temàtiques de la UPC] ,Cross section ,Reaccions nuclears ,Resonance ,Neutron temperature ,Time of flight ,Neutron capture ,Nuclear reactions - Abstract
The neutron capture cross section of 58 Ni was measured at the neutron time of flight facility n_TOF at CERN, from 27 meV to 400 keV neutron energy. Special care has been taken to identify all the possible sources of background, with the so-called neutron background obtained for the first time using high-precision GEANT4 simulations. The energy range up to 122 keV was treated as the resolved resonance region, where 51 resonances were identified and analyzed by a multilevel R -matrix code SAMMY. Above 122 keV the code SESH was used in analyzing the unresolved resonance region of the capture yield. Maxwellian averaged cross sections were calculated in the temperature range of kT = 5 – 100 keV, and their astrophysical implications were investigated.
- Published
- 2015