Bereiche | Tage | Auswahl | Suche | Downloads | Hilfe
HK: Fachverband Hadronen und Kerne
HK 50: Nuclear Astrophysics
HK 50.3: Vortrag
Mittwoch, 18. März 2009, 14:45–15:00, H-ZO 60
Strength, decay branching ratios, and angular distribution of the 0.987 MeV resonance in the 14N(p,γ)15O reaction — •Michele Marta1, Daniel Bemmerer1, Roland Beyer1, Carlo Broggini2, Antonio Caciolli2, Martin Erhard1, Zsolt Fülöp3, Eckart Grosse1, György Gyürky3, Roland Hannaske1, Arnd Rudolf Junghans1, Roberto Menegazzo2, Chithra Nair1, Roland Schwengner1, Tamas Szücs3, Erik Trompler1, Andreas Wagner1, and Dmitry Yakorev1 — 1Forschungszentrum Dresden-Rossendorf (FZD), Dresden, Germany — 2INFN Sezione di Padova, Padova, Italy — 3ATOMKI, Debrecen, Hungary
The 14N(p,γ)15O reaction controls the rate of the hydrogen burning CNO cycle. This reaction has recently been re-studied at E < 500 keV at different facilities, including LUNA. However, also data at higher energy play a role in determining the extrapolated cross section in the R-matrix framework. Here we report on a new measurement of the absolute strength, decay branching ratio, and angular distribution of the E = 0.987 MeV (Ex = 8.284 MeV) resonance carried out at the high-current FZD Tandetron. — This work has been supported in part by the European Union (FP6 AIM RITA 025646).