49 citations · 116 across the 6 of their papers we have counts for
6 papers
Astrophysical S-factor of the reaction at 0.4 -- 1.3\,MeV
L. Wagner, S. Akhmadaliev, M. Anders +18
The reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowl…
Absolute hydrogen depth profiling using the resonant H(N,)C nuclear reaction
Tobias P. Reinhardt, Shavkat Akhmadaliev, Daniel Bemmerer +2
Resonant nuclear reactions are a powerful tool for the determination of the amount and profile of hydrogen in thin layers of material. Usually, this tool requires the use of a stan…
Silicon photomultiplier readout of a monolithic 27055 cm plastic scintillator bar for time of flight applications
Tobias P. Reinhardt, Stefan Gohl, Stefan Reinicke +8
The detection of 200-1000 MeV neutrons requires large amounts, 100 cm, of detector material because of the long nuclear interaction length of these particles. In the example…
Determination of gamma-ray widths in N using nuclear resonance fluorescence
T. Szücs, D. Bemmerer, A. Caciolli +9
The stable nucleus N is the mirror of O, the bottleneck in the hydrogen burning CNO cycle. Most of the N level widths below the proton emission threshold are k…
Cosmic-ray induced background intercomparison with actively shielded HPGe detectors at underground locations
T. Szücs, D. Bemmerer, T. P. Reinhardt +6
The main background above 3\,MeV for in-beam nuclear astrophysics studies with -ray detectors is caused by cosmic-ray induced secondaries. The two commonly used suppression meth…
Nuclear deformation and neutron excess as competing effects for pygmy dipole strength
R. Massarczyk, R. Schwengner, F. Dönau +27
The electromagnetic dipole strength below the neutron-separation energy has been studied for the xenon isotopes with mass numbers A = 124, 128, 132, and 134 in nuclear resonance fl…