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Recent results of the 14N(p,γ)15O measurement at LUNA
Università di Genova.
Centre de Recherches du Cyclotron, Universit¶e Catholique de Louvain, Louvain-la-Neuve.
Institut für Atomare Physik und Fachdidaktik, Technische Universität Berlin.
Università Degli Studi di Milano and INFN.
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Number of Authors: 332005 (English)In: Nuclear Physics A, ISSN 0375-9474, E-ISSN 1873-1554, Vol. 758, no 1-4 SPEC. ISS., p. 383C-386CArticle in journal (Refereed) Published
Abstract [en]

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 4π BGO summing crystal has been used and the total S-factor has been measured down to Eb = 80 keV. © 2005 Elsevier B.V. All rights reserved.

Place, publisher, year, edition, pages
2005. Vol. 758, no 1-4 SPEC. ISS., p. 383C-386C
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Experimental Physics
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URN: urn:nbn:se:ltu:diva-6165DOI: 10.1016/j.nuclphysa.2005.05.069ISI: 000230660500082Scopus ID: 2-s2.0-20944443307Local ID: 45f5313b-1e63-49b0-82c0-b58e5cd379a9OAI: oai:DiVA.org:ltu-6165DiVA, id: diva2:979042
Note

Upprättat; 2005; 20141216 (albvom)

Available from: 2016-09-29 Created: 2016-09-29 Last updated: 2018-10-04Bibliographically approved

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Vomiero, Alberto

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