34 citations · 125 across the 12 of their papers we have counts for
8 papers · 1 filter
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 ambient neutron flux and spectral distribution at the Canfranc Underground Laboratory
S. E. A. Orrigo, J. L. Tain, N. Mont-Geli +13
We report on the measurement of the ambient neutron flux and its energy distribution over a broad range of neutron energies, conducted in Hall A of the Canfranc Underground Laborat…
Long-term evolution of the neutron rate at the Canfranc Underground Laboratory
S. E. A. Orrigo, J. L. Tain, N. Mont-Geli +14
We report results on the long-term variation of the neutron counting rate at the Canfranc Underground Laboratory, of importance for several low-background experiments installed the…
Measurement of the neutron flux at the Canfranc Underground Laboratory with HENSA
S. E. A. Orrigo, J. L. Tain, N. Mont-Geli +14
We have performed a long-term measurement of the neutron flux with the High Efficiency Neutron Spectrometry Array HENSA in the Hall A of the Canfranc Underground Laboratory. The Ha…
First results from the HENSA/ANAIS collaboration at the Canfranc Underground Laboratory
N Mont-Geli, A Tarifeño-Saldivia, S E A Orrigo +24
The HENSA/ANAIS collaboration aims for the precise determination of the neutron flux that could affect ANAIS-112, an experiment looking for the dark matter annual modulation using…
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…
Background in -ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory
T. Szücs, D. Bemmerer, D. Degering +7
The relevant interaction energies for astrophysical radiative capture reactions are very low, much below the repulsive Coulomb barrier. This leads to low cross sections, low counti…
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…