New determination of the 12C(α, γ)16O reaction rate from γ-ray angular distribution measurements-Reference-Cited by-同舟云学术

New determination of the 12C(α, γ)16O reaction rate from γ-ray angular distribution measurements

Published:2005-04 Issue: Volume:752 Page:514-521
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Hammer J.W.,Fey M.,Kunz R.,Kiener J.,Tatischeff V.,Haas F.,Weil J.L.,Assunção M.,Beck C.,Boukari-Pelissie C.,Coc A.,Correia J.J.,Courtin S.,Fleurot F.,Galanopoulos E.,Grama C.,Hammache F.,Harissopulos S.,Korichi A.,Krmpotić E.,Le Du D.,Lopez-Martens A.,Malcherek D.,Meunier R.,Papka P.,Paradellis T.,Rousseau M.,Rowley N.,Staudt G.,Szilner S.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference25 articles.

1. Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics

2. M. Fey, PhD thesis, Stuttgart, Germany (2004), http://elib.uni-stuttgart.de/opus/volltexte/2004/1683/

3. Astrophysical Reaction Rate of12C(α, γ)16O

4. A compilation of charged-particle induced thermonuclear reaction rates

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