TY - JOUR
T1 - Accelerator mass spectrometry measurement of the reaction Cl 35 (n,γ) Cl 36 at keV energies
AU - Pavetich, Stefan
AU - Wallner, Anton
AU - Martschini, Martin
AU - Akhmadaliev, Shavkat
AU - Dillmann, Iris
AU - Fifield, Keith
AU - Halfon, Shlomi
AU - Heftrich, Tanja
AU - Käppeler, Franz
AU - Lederer-Woods, Claudia
AU - Merchel, Silke
AU - Paul, Michael
AU - Reifarth, René
AU - Rugel, Georg
AU - Steier, Peter
AU - Tessler, Moshe
AU - Tims, Stephen
AU - Weigand, Mario
AU - Weissman, Leo
N1 - Publisher Copyright:
© 2019 American Physical Society.
PY - 2019/1/8
Y1 - 2019/1/8
N2 - The nuclide Cl35 can act as a minor "neutron poison" in the stellar slow neutron capture process. Neutron activation combined with accelerator mass spectrometry (AMS) was applied to measure the (n,γ) cross section of Cl35 for neutron spectra simulating Maxwell-Boltzmann distributions of kT≈30 and 40 keV. The neutron activations were performed at the Karlsruhe Van de Graaff accelerator and at the superconducting linear accelerator of the Soreq Applied Research Accelerator Facility utilizing the Li7(p,n)Be7 reaction. AMS measurements of the irradiated samples were performed at the 3 MV Vienna Environmental Research Accelerator, the 6 MV tandem accelerator at the Dresden AMS facility, and the 14 UD tandem accelerator of the Australian National University in Canberra. Our method is independent of previous measurements. For an energy of kT=30keV, we report a Maxwellian averaged cross section of 8.33(32) mb. Using this new value in stellar isotopic abundance calculations, minor changes for the abundances of Cl35, Cl36, and S36 are derived.
AB - The nuclide Cl35 can act as a minor "neutron poison" in the stellar slow neutron capture process. Neutron activation combined with accelerator mass spectrometry (AMS) was applied to measure the (n,γ) cross section of Cl35 for neutron spectra simulating Maxwell-Boltzmann distributions of kT≈30 and 40 keV. The neutron activations were performed at the Karlsruhe Van de Graaff accelerator and at the superconducting linear accelerator of the Soreq Applied Research Accelerator Facility utilizing the Li7(p,n)Be7 reaction. AMS measurements of the irradiated samples were performed at the 3 MV Vienna Environmental Research Accelerator, the 6 MV tandem accelerator at the Dresden AMS facility, and the 14 UD tandem accelerator of the Australian National University in Canberra. Our method is independent of previous measurements. For an energy of kT=30keV, we report a Maxwellian averaged cross section of 8.33(32) mb. Using this new value in stellar isotopic abundance calculations, minor changes for the abundances of Cl35, Cl36, and S36 are derived.
UR - http://www.scopus.com/inward/record.url?scp=85059870330&partnerID=8YFLogxK
U2 - 10.1103/PhysRevC.99.015801
DO - 10.1103/PhysRevC.99.015801
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AN - SCOPUS:85059870330
SN - 2469-9985
VL - 99
JO - Physical Review C
JF - Physical Review C
IS - 1
M1 - 015801
ER -