Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project
This contribution is focused on the STELLA project (STELlar LAboratory), which aims at the measurement of fusion cross sections between light heavy ions like 12C+12C, 12C+16O or 16O+16O at deep subbarrier energies. The gamma-particle coincidence technique is used in order to reduce background contri...
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Online Access: | https://doi.org/10.1051/epjconf/201716300018 |
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doaj-3d7ed80e0cc14bb8b8b8449b30abae0c2021-08-02T09:38:47ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011630001810.1051/epjconf/201716300018epjconf_fusion2017_00018Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA projectFruet GuillaumeCourtin SandrineJenkins David G.Heine MarcelMontanari DanieleMorris Luke G.Adsley PhilipBeck ChristianDella Negra SergeHaas FlorentHammache FairouzKirsebom Oliver S.Meyer AnneRegan Patrick H.Rudiger Matthiasde Séréville NicolasStodel ChristelleThis contribution is focused on the STELLA project (STELlar LAboratory), which aims at the measurement of fusion cross sections between light heavy ions like 12C+12C, 12C+16O or 16O+16O at deep subbarrier energies. The gamma-particle coincidence technique is used in order to reduce background contributions that become dominant for measurements in the nanobarn regime. The experimental setup composed of an ultra high vacuum reaction chamber, a set of 3 silicon strip detectors, up to 36 LaBr3(Ce) scintillators from the UK FATIMA collaboration, and a fast rotating target system will be described. The 12C+12C fusion reaction has been studied from Elab = 11 to 5.6 MeV using STELLA at the Andromède facility in Orsay, France. Preliminary commissioning results are presented in this article.https://doi.org/10.1051/epjconf/201716300018 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Fruet Guillaume Courtin Sandrine Jenkins David G. Heine Marcel Montanari Daniele Morris Luke G. Adsley Philip Beck Christian Della Negra Serge Haas Florent Hammache Fairouz Kirsebom Oliver S. Meyer Anne Regan Patrick H. Rudiger Matthias de Séréville Nicolas Stodel Christelle |
spellingShingle |
Fruet Guillaume Courtin Sandrine Jenkins David G. Heine Marcel Montanari Daniele Morris Luke G. Adsley Philip Beck Christian Della Negra Serge Haas Florent Hammache Fairouz Kirsebom Oliver S. Meyer Anne Regan Patrick H. Rudiger Matthias de Séréville Nicolas Stodel Christelle Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project EPJ Web of Conferences |
author_facet |
Fruet Guillaume Courtin Sandrine Jenkins David G. Heine Marcel Montanari Daniele Morris Luke G. Adsley Philip Beck Christian Della Negra Serge Haas Florent Hammache Fairouz Kirsebom Oliver S. Meyer Anne Regan Patrick H. Rudiger Matthias de Séréville Nicolas Stodel Christelle |
author_sort |
Fruet Guillaume |
title |
Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project |
title_short |
Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project |
title_full |
Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project |
title_fullStr |
Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project |
title_full_unstemmed |
Fusion cross section measurements of astrophysical interest for light heavy ions systems within the STELLA project |
title_sort |
fusion cross section measurements of astrophysical interest for light heavy ions systems within the stella project |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2017-01-01 |
description |
This contribution is focused on the STELLA project (STELlar LAboratory), which aims at the measurement of fusion cross sections between light heavy ions like 12C+12C, 12C+16O or 16O+16O at deep subbarrier energies. The gamma-particle coincidence technique is used in order to reduce background contributions that become dominant for measurements in the nanobarn regime.
The experimental setup composed of an ultra high vacuum reaction chamber, a set of 3 silicon strip detectors, up to 36 LaBr3(Ce) scintillators from the UK FATIMA collaboration, and a fast rotating target system will be described. The 12C+12C fusion reaction has been studied from Elab = 11 to 5.6 MeV using STELLA at the Andromède facility in Orsay, France. Preliminary commissioning results are presented in this article. |
url |
https://doi.org/10.1051/epjconf/201716300018 |
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