New γ-ray production cross sections for the 4.439 and 6.129 MeV lines of 12C and 16O. Astrophysical implications

S. Ouichaoui, Y. Rahma, J. Kiener, E. A. Lawrie, J. J. Lawrie, V. Tatischeff, A. Belhout, D. Moussa, W. Yahia-Cherif, H. Benhabiles-Mezhoud, T. D. Bucher, T. R.S. Dinoko, A. Chafa, J. L. Conradie, S. Damache, M. Debabi, I. Deloncle, J. L. Easton, M. Fouka, C. HamadacheF. Hammache, P. Jones, B. V. Kheswa, N. A. Khumalo, T. Lamula, S. N.T. Majola, J. Ndayishimye, D. Negi, S. P. Noncolela, S. Ouziane, P. Papka, S. Peterson, M. Kumar Raju, V. Ramanathan, B. M. Rebeiro, N. de Séréville, J. F. Sharpey-Schafer, O. Shirinda, M. Wiedeking, S. Wyngaardt

Research output: Contribution to journalConference articlepeer-review

Abstract

Gamma-ray line production cross sections from nuclear reactions induced by 30-200 MeV protons on natC and Mylar targets have been measured at the SSC facility of iThemba LABS. Results for the 4.439 and 6.129 MeV prominent lines of 12C and 16O of astrophysical concern are reported and discussed.

Original languageEnglish
Article number012099
JournalJournal of Physics: Conference Series
Volume2586
Issue number1
DOIs
Publication statusPublished - 2023
Event28th International Nuclear Physics Conference, INPC 2022 - Cape Town, South Africa
Duration: 11 Sept 202216 Sept 2022

ASJC Scopus subject areas

  • General Physics and Astronomy

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