35 citations · 210 across the 14 of their papers we have counts for
13 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…
Online Bayesian Optimization for Beam Alignment in the SECAR Recoil Mass Separator
Sara A. Miskovich, Fernando Montes, Georg P. A. Berg +10
The SEparator for CApture Reactions (SECAR) is a next-generation recoil separator system at the Facility for Rare Isotope Beams (FRIB) designed for the direct measurement of captur…
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…
Resonance strengths in the 14N(p,gamma)15O astrophysical key reaction measured with activation
Gy. Gyürky, Z. Halász, G. G. Kiss +7
The 14N(p,gamma)15O reaction plays a vital role in various astrophysical scenarios. Its reaction rate must be accurately known in the present era of high precision astrophysics. Th…
The muon intensity in the Felsenkeller shallow underground laboratory
F. Ludwig, L. Wagner, T. Al-Abdullah +7
The muon intensity and angular distribution in the shallow-underground laboratory Felsenkeller in Dresden, Germany have been studied using a portable muon detector based on the clo…
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…
Double electron capture searches in Se
B. Lehnert, T. Wester, D. Degering +3
A search for various double electron capture modes of Se has been performed using an ultralow background Ge-detector in the Felsenkeller laboratory, Germany. Especially for…
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…
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…
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…