35 citations · 104 across the 6 of their papers we have counts for
7 papers
The 3He(α,γ)7Be γ-ray angular distribution: measured, and calculated by effective field theory
S. Turkat, P. Hempel, X. Zhang +26
The 3He(alpha,gamma)7Be reaction takes place in several distinct astrophysical scenarios. First, in solar hydrogen burning, 3He(alpha,gamma)7Be controls the competition between the…
Measurement of the H()He S-factor at 265-1094keV
S. Turkat, S. Hammer, E. Masha +14
Recent astronomical data have provided the primordial deuterium abundance with percent precision. As a result, Big Bang nucleosynthesis may provide a constraint on the universal ba…
The new Felsenkeller 5 MV underground accelerator
Daniel Bemmerer, Thomas E. Cowan, Alexander Domula +18
The field of nuclear astrophysics is devoted to the study of the creation of the chemical elements. By nature, it is deeply intertwined with the physics of the Sun. The nuclear rea…
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…
Progress of the Felsenkeller shallow-underground accelerator for nuclear astrophysics
D. Bemmerer, F. Cavanna, T. E. Cowan +15
Low-background experiments with stable ion beams are an important tool for putting the model of stellar hydrogen, helium, and carbon burning on a solid experimental foundation. The…
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…
Strengths of the resonances at 436, 479, 639, 661, and 1279 keV in the Ne(p,)Na reaction
Rosanna Depalo, Francesca Cavanna, Federico Ferraro +11
The Ne(p,)Na reaction is included in the neon-sodium cycle of hydrogen burning. A number of narrow resonances in the Gamow window dominates the thermonuclear react…