$$^{74}$$Ge($$n,\gamma $$) cross section below 70 keV measured at n_TOF CERN

Media type: E-Article
Title: $$^{74}$$Ge($$n,\gamma $$) cross section below 70 keV measured at n_TOF CERN
Contributor: Lederer-Woods, C.; Aberle, O.; Andrzejewski, J.; Audouin, L.; Bécares, V.; Bacak, M.; Balibrea, J.; Barbagallo, M.; Barros, S.; Battino, U.; Bečvář, F.; Beinrucker, C.; Berthoumieux, E.; Billowes, J.; Bosnar, D.; Brugger, M.; Caamaño, M.; Calviño, F.; Calviani, M.; Cano-Ott, D.; Cardella, R.; Casanovas, A.; Castelluccio, D. M.; Cerutti, F.; [...]
imprint: Springer Science and Business Media LLC, 2022
Published in: The European Physical Journal A
Language: English
DOI: 10.1140/epja/s10050-022-00878-5
ISSN: 1434-601X
Keywords: Nuclear and High Energy Physics
Origination:
Footnote:
Description: <jats:title>Abstract</jats:title><jats:p>Neutron capture reaction cross sections on <jats:inline-formula><jats:alternatives><jats:tex-math>$$^{74}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>74</mml:mn> </mml:msup> </mml:math></jats:alternatives></jats:inline-formula>Ge are of importance to determine <jats:inline-formula><jats:alternatives><jats:tex-math>$$^{74}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>74</mml:mn> </mml:msup> </mml:math></jats:alternatives></jats:inline-formula>Ge production during the astrophysical slow neutron capture process. We present new resonance data on <jats:inline-formula><jats:alternatives><jats:tex-math>$$^{74}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>74</mml:mn> </mml:msup> </mml:math></jats:alternatives></jats:inline-formula>Ge(<jats:inline-formula><jats:alternatives><jats:tex-math>$$n,\gamma $$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>n</mml:mi> <mml:mo>,</mml:mo> <mml:mi>γ</mml:mi> </mml:mrow> </mml:math></jats:alternatives></jats:inline-formula>) reactions below 70 keV neutron energy. We calculate Maxwellian averaged cross sections, combining our data below 70 keV with evaluated cross sections at higher neutron energies. Our stellar cross sections are in agreement with a previous activation measurement performed at Forschungszentrum Karlsruhe by Marganiec et al., once their data has been re-normalised to account for an update in the reference cross section used in that experiment.</jats:p>

Search in field:

Recently searched for: