Cargando…

Neutron Capture Cross Section for $^{10}\mathrm{Be}$

The determination of the involved reaction cross sections is essential for the understanding of how the big bang nucleosynthesis and nuclear reactions in stars contribute to the observed abundances. One of those, which has not been measured so far, is the $^{10}\mathrm{Be(n,\gamma)}$ cross section....

Descripción completa

Detalles Bibliográficos
Autores principales: Volknandt, M, Eberhardt, K, Endres, A, Erbacher, P, Fix, M, Göbel, K, Heftrich, T, Heinitz, S, Hrivula, E, Junghans, A, Käppeler, F, Kivel, N, Langer, C, Mengoni, A, Reifarth, R, Schmidt, S, Schumann, D, Thomas, B, Veltum, D, Weigand, M, Wiehl, N, Wolf, C
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1742-6596/1668/1/012048
http://cds.cern.ch/record/2749819
Descripción
Sumario:The determination of the involved reaction cross sections is essential for the understanding of how the big bang nucleosynthesis and nuclear reactions in stars contribute to the observed abundances. One of those, which has not been measured so far, is the $^{10}\mathrm{Be(n,\gamma)}$ cross section. A $^{10}\mathrm{BeO}$ sample, provided by PSI Villigen, was irradiated in a cyclic activation at the TRIGA reactor in Mainz. The characteristic $\gamma$-rays following the decay of $^{11}\mathrm{Be}$ were measured using $\mathrm{LaBr_3}$ scintillation detectors. The thermal neutron cross section and the resonance integral were experimentally determined for the first time.