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The (n, $\gamma$) cross sections of short-living s-process branching points

An experimental method to determine the (n,g) cross section of short-living s-process branching points using data of the inverse (g,n) reaction is presented. The method was used to observe the branching point nucleus 95Zr because the elemental abundance patterns corresponding to this branching point...

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Detalles Bibliográficos
Autores principales: Sonnabend, Kerstin, Mengoni, A., Mohr, P., Rauscher, T., Vogt, K., Zilges, A.
Lenguaje:eng
Publicado: 2004
Materias:
Acceso en línea:https://dx.doi.org/10.1063/1.1737142
http://cds.cern.ch/record/732639
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author Sonnabend, Kerstin
Mengoni, A.
Mohr, P.
Rauscher, T.
Vogt, K.
Zilges, A.
author_facet Sonnabend, Kerstin
Mengoni, A.
Mohr, P.
Rauscher, T.
Vogt, K.
Zilges, A.
author_sort Sonnabend, Kerstin
collection CERN
description An experimental method to determine the (n,g) cross section of short-living s-process branching points using data of the inverse (g,n) reaction is presented. The method was used to observe the branching point nucleus 95Zr because the elemental abundance patterns corresponding to this branching point cannot be reproduced by full stellar models and a possible error source is the neutron capture cross section of 95Zr. The analysis of the experiment is still under progress, we will outline the current status in this manuscript.
id cern-732639
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2004
record_format invenio
spelling cern-7326392019-09-30T06:29:59Zdoi:10.1063/1.1737142http://cds.cern.ch/record/732639engSonnabend, KerstinMengoni, A.Mohr, P.Rauscher, T.Vogt, K.Zilges, A.The (n, $\gamma$) cross sections of short-living s-process branching pointsAstrophysics and AstronomyAn experimental method to determine the (n,g) cross section of short-living s-process branching points using data of the inverse (g,n) reaction is presented. The method was used to observe the branching point nucleus 95Zr because the elemental abundance patterns corresponding to this branching point cannot be reproduced by full stellar models and a possible error source is the neutron capture cross section of 95Zr. The analysis of the experiment is still under progress, we will outline the current status in this manuscript.astro-ph/0404552oai:cds.cern.ch:7326392004
spellingShingle Astrophysics and Astronomy
Sonnabend, Kerstin
Mengoni, A.
Mohr, P.
Rauscher, T.
Vogt, K.
Zilges, A.
The (n, $\gamma$) cross sections of short-living s-process branching points
title The (n, $\gamma$) cross sections of short-living s-process branching points
title_full The (n, $\gamma$) cross sections of short-living s-process branching points
title_fullStr The (n, $\gamma$) cross sections of short-living s-process branching points
title_full_unstemmed The (n, $\gamma$) cross sections of short-living s-process branching points
title_short The (n, $\gamma$) cross sections of short-living s-process branching points
title_sort (n, $\gamma$) cross sections of short-living s-process branching points
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1063/1.1737142
http://cds.cern.ch/record/732639
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