activity
20052024
most citedFirst measurement of the 14N(p,gamma)15O cross section down to 70 keV

124 citations · 373 across the 8 of their papers we have counts for

collaborators

8 papers

cond-mat.mtrl-sci2024★ 2 cited

On the influence of annealing on the compositional and crystallographic properties of sputtered Li-Al-O thin films

Florian Lourens, Detlef Rogalla, Ellen Suhr +1

A Li-Al-O thin film materials library, deposited by inert magnetron sputtering and post-deposition annealing in O2 atmosphere, was used to study the effects of different annealing…

cond-mat.mtrl-sci2022

Unusual phase formation in reactively sputtered La-Co-O perovskite thin films

Tobias H. Piotrowiak, Rico Zehl, Ellen Suhr +4

La-based perovskites are a versatile class of materials that are of interest for solid oxide fuel cells and electrocatalytic water splitting. During fabrication of composition spre…

quant-ph2021★ 68 cited

Coherence of a charge stabilised tin-vacancy spin in diamond

Johannes Görlitz, Dennis Herrmann, Philipp Fuchs +8

Quantum information processing (QIP) with solid state spin qubits strongly depends on the efficient initialisation of the qubit's desired charge state. While the negatively charged…

nucl-ex2015★ 29 cited

Measurement of the 187Re(α,n)190Ir reaction cross section at sub-Coulomb energies using the Cologne Clover Counting Setup

P. Scholz, A. Endres, A. Hennig +10

Uncertainties in adopted models of particle+nucleus optical-model potentials directly influence the accuracy in the theoretical predictions of reaction rates as they are needed for…

quant-ph2010★ 4 cited

Single-photon emission from Ni-related color centers in CVD diamond

David Steinmetz, Elke Neu, Christian Hepp +5

Color centers in diamond are very promising candidates among the possible realizations for practical single-photon sources because of their long-time stable emission at room temper…

nucl-ex2006★ 124 cited

First measurement of the 14N(p,gamma)15O cross section down to 70 keV

A. Lemut, D. Bemmerer, F. Confortola +28

In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate is determined by the slowest process, the 14N(p,gamma)15O reaction. Deep underg…