| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9850980 | Nuclear Physics A | 2005 | 4 Pages |
Abstract
The 14N(p,γ)15O reaction has been investigated by LUNA at the National Laboratory of Gran Sasso (LNGS) using two different techniques. The first study has been performed using a solid target and detecting the γ-rays coming from the single transitions with a HPGe detector in very close geometry to the target. In a second phase a windowless gas target sorrounded by a nearly 4Ï BGO summing crystal has been used and the total S-factor has been measured down to Eb=80 keV.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
H. Costantini, C. Angulo, D. Bemmerer, R. Bonetti, C. Broggini, F. Confortola, P. Corvisiero, J. Cruz, P. Descouvemont, A. Formicola, Z. Fülop, G. Gervino, A. Guglielmetti, C. Gustavino, G. Gyürky, G. Imbriani, A.P. Jesus, M. Junker, S. Zavatarelli,