English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/117964
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:


He-3(alpha, gamma) Be-7 cross section measured using complementary techniques.

AuthorsCarmona Gallardo, M. ; García Borge, María José ; Davids, B.; Fulton, B.R.; Hass, M.; Nara Singh, B.S.; Ruiz, C.; Tengblad, Olof
Issue Date20-Mar-2014
PublisherEDP Sciences
CitationEPJ Web of Conferences 66: 07003 (2014)
AbstractThe astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standard Model and in the Big Bang Nucleosynthesis scenario. The advances from two recent experiments performed using complementary techniques at center of mass (C.M.) energies between 1 and 3 MeV are discussed.
DescriptionINPC 2013 – International Nuclear Physics Conference; 4 pags.; 3 figs.; Open Access funded by Creative Commons Atribution Licence 2.0
Publisher version (URL)http://dx.doi.org/10.1051/epjconf/20146607003
Identifiersdoi: 10.1051/epjconf/20146607003
issn: 2100-014X
Appears in Collections:(CFMAC-IEM) Artículos
Files in This Item:
File Description SizeFormat 
MCarmona.pdf1,06 MBAdobe PDFThumbnail
Show full item record
Review this work

Related articles:

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.