The 14N(p, γ)15O measurement at low energy

Confortola, F. and Bemmerer, D. and Bonetti, R. and Broggini, C. and Corvisiero, P. and Costantini, H. and Cruz, J. and Formicola, A. and Fülop, Z. and Gervino, G. and Guglielmetti, A. and Gustavino, C. and Gyürky, G. and Imbriani, G. and Jesus, A. P. and Junker, M. and Lemut, A. and Menegazzo, R. and Prati, P. and Roca, V. and Rolfs, C. and Romano, M. and Rossi Alvarez, C. and Schümann, F. and Somorjai, E. and Straniero, O. and Strieder, F. and Terrasi, F. and Trautvetter, H. P. and Zavatarelli, S. (2004) The 14N(p, γ)15O measurement at low energy. Il nuovo cimento C, 27 (5). pp. 423-427. ISSN 1826-9885

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The 14N(p, γ)15O reaction has been investigated by the LUNA experiment at the National Laboratory of Gran Sasso (LNGS). This study has been performed with two different technical set-ups. The first one, suitable for the detection of γ-rays coming from the single transitions, has been realized with a HPGe detector and a solid target. The second has been made of a BGO summing Crystal as a detector and a windowless gas target. The high-detection efficiency and the target purity of the gas target set-up allowed to measure the total S-factor down to Ec.m. = 71 keV.

Item Type: Article
Uncontrolled Keywords: Resonance reactions ; Direct reactions ; Hydrostatic stellar nucleosynthesis
Subjects: 500 Scienze naturali e Matematica > 530 Fisica
Depositing User: Marina Spanti
Date Deposited: 14 Mar 2020 12:02
Last Modified: 14 Mar 2020 12:02

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