activity
20022020
most citedIsospin Character of the Pygmy Dipole Resonance in 124Sn

173 citations · 629 across the 20 of their papers we have counts for

collaborators

20 papers

nucl-ex2020★ 8 cited

Structure of high-lying levels populated in the Y Zr decay

K. R. Mashtakov, V. Yu. Ponomarev, M. Scheck +32

The nature of levels of Zr below the -decay value of Y has been investigated in high-resolution -ray spectroscopy following the decay as wel…

physics.ins-det2016★ 3 cited

Behavior of a trapezoid-based data acquisition system up to 100 kHz and beyond

Stefan Schmidt, Tanja Heftrich, Jan Glorius +8

In this work, we investigated the ability of a high-purity germanium detector connected to a trapezoid-filter-based data acquisition system to reliably record signals in spite of h…

astro-ph.SR2016★ 24 cited

Sensitivity study for s process nucleosynthesis in AGB stars

A. Koloczek, B. Thomas, J. Glorius +6

In this paper we present a large-scale sensitivity study of reaction rates in the main component of the process. The aim of this study is to identify all rates, which have a gl…

astro-ph.IM2015★ 14 cited

Nucleosynthesis simulations for the production of the p-nuclei Mo and Mo in a Supernova type II model

Kathrin Göbel, Jan Glorius, Alexander Koloczek +4

We present a nucleosynthesis sensitivity study for the -process in a Supernova type II model within the NuGrid research platform. The simulations aimed at identifying the releva…

nucl-ex2015★ 1 cited

Measurements of neutron-induced reactions in inverse kinematics and applications to nuclear astrophysics

René Reifarth, Yuri A. Litvinov, Anne Endres +7

Neutron capture cross sections of unstable isotopes are important for neutron-induced nucleosynthesis as well as for technological applications. A combination of a radioactive beam…

nucl-ex2015★ 8 cited

The thermal neutron capture cross section of the radioactive isotope Fe

T. Heftrich, M. Bichler, R. Dressler +20

50% of the heavy element abundances are produced via slow neutron capture reactions in different stellar scenarios. The underlying nucleosynthesis models need the input of neutron…