Neutron activations for lower s-process temperatures

The slow neutron capture process produces heavy elements in different stellar sites at different temperatures. Neutron capture cross sections for stellar temperatures between kBT = 5 keV and kBT = 100 keV are crucial for a quantitative understanding of the s-process abundance distribution. Over the...

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Main Authors: Heftrich Tanja, Al-Khasawleh Kafa, Borzek Sandra, Brückner Benjamin, Dellmann Sophia Florence, Dogan Ozan Can, El Mard Asmaa, Erbacher Philipp, Gail Madeleine, Göbel Kathrin, Habermehl Fabian, Heybeck Benedict, Kisselbach Timo, Kurtulgil Deniz, Mourad Rim, Reich Markus, Reifarth René, Sheriff Silas, Staab Tom, Volknandt Meiko, Weigand Mario
Format: Article
Language:English
Published: EDP Sciences 2023-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_06011.pdf
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author Heftrich Tanja
Al-Khasawleh Kafa
Borzek Sandra
Brückner Benjamin
Dellmann Sophia Florence
Dogan Ozan Can
El Mard Asmaa
Erbacher Philipp
Gail Madeleine
Göbel Kathrin
Habermehl Fabian
Heybeck Benedict
Kisselbach Timo
Kurtulgil Deniz
Mourad Rim
Reich Markus
Reifarth René
Sheriff Silas
Staab Tom
Volknandt Meiko
Weigand Mario
author_facet Heftrich Tanja
Al-Khasawleh Kafa
Borzek Sandra
Brückner Benjamin
Dellmann Sophia Florence
Dogan Ozan Can
El Mard Asmaa
Erbacher Philipp
Gail Madeleine
Göbel Kathrin
Habermehl Fabian
Heybeck Benedict
Kisselbach Timo
Kurtulgil Deniz
Mourad Rim
Reich Markus
Reifarth René
Sheriff Silas
Staab Tom
Volknandt Meiko
Weigand Mario
author_sort Heftrich Tanja
collection DOAJ
description The slow neutron capture process produces heavy elements in different stellar sites at different temperatures. Neutron capture cross sections for stellar temperatures between kBT = 5 keV and kBT = 100 keV are crucial for a quantitative understanding of the s-process abundance distribution. Over the last decade activation measurements were performed at the Goethe University Frankfurt to study cross sections at a temperature of kBT = 25 keV. We developed a new method to measure neutron capture cross sections at kBT = 6 keV.
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spelling doaj.art-3dcda5e898804a158fd3726b0e88301a2023-04-07T09:02:03ZengEDP SciencesEPJ Web of Conferences2100-014X2023-01-012790601110.1051/epjconf/202327906011epjconf_npa-x2023_06011Neutron activations for lower s-process temperaturesHeftrich Tanja0Al-Khasawleh Kafa1Borzek Sandra2Brückner Benjamin3Dellmann Sophia Florence4Dogan Ozan Can5El Mard Asmaa6Erbacher Philipp7Gail Madeleine8Göbel Kathrin9Habermehl Fabian10Heybeck Benedict11Kisselbach Timo12Kurtulgil Deniz13Mourad Rim14Reich Markus15Reifarth René16Sheriff Silas17Staab Tom18Volknandt Meiko19Weigand Mario20Goethe University FrankfurtJordan Atomic Energy Commission/Jordan Research and Training ReactorGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtFacility for Antiproton and Ion Research in Europe GmbH (FAIR GmbH)Goethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtGoethe University FrankfurtThe slow neutron capture process produces heavy elements in different stellar sites at different temperatures. Neutron capture cross sections for stellar temperatures between kBT = 5 keV and kBT = 100 keV are crucial for a quantitative understanding of the s-process abundance distribution. Over the last decade activation measurements were performed at the Goethe University Frankfurt to study cross sections at a temperature of kBT = 25 keV. We developed a new method to measure neutron capture cross sections at kBT = 6 keV.https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_06011.pdf
spellingShingle Heftrich Tanja
Al-Khasawleh Kafa
Borzek Sandra
Brückner Benjamin
Dellmann Sophia Florence
Dogan Ozan Can
El Mard Asmaa
Erbacher Philipp
Gail Madeleine
Göbel Kathrin
Habermehl Fabian
Heybeck Benedict
Kisselbach Timo
Kurtulgil Deniz
Mourad Rim
Reich Markus
Reifarth René
Sheriff Silas
Staab Tom
Volknandt Meiko
Weigand Mario
Neutron activations for lower s-process temperatures
EPJ Web of Conferences
title Neutron activations for lower s-process temperatures
title_full Neutron activations for lower s-process temperatures
title_fullStr Neutron activations for lower s-process temperatures
title_full_unstemmed Neutron activations for lower s-process temperatures
title_short Neutron activations for lower s-process temperatures
title_sort neutron activations for lower s process temperatures
url https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_06011.pdf
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