Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies

A cross section measurement employing a direct 16O detection method for the reaction energies from Ecm = 2.4 to 0.7 MeV is planned at Kyushu University Tandem Laboratory (KUTL). To perform this experiment and to obtain quantitative information about the cross section to within an error of 10%, we ha...

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Main Authors: Fujita Kunihiro, Yamaguchi Hiroyuki, Ban Tadahiko, Hamamoto Kenichi, Narikiyo Yoshihiro, Tao Nariaki, Sagara Kenshi
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20159303005
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spelling doaj-18f803a5b2e546c3a33ed66b6e3c99702021-08-02T01:48:17ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01930300510.1051/epjconf/20159303005epjconf_cgs2015_03005Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar EnergiesFujita Kunihiro0Yamaguchi Hiroyuki1Ban Tadahiko2Hamamoto Kenichi3Narikiyo Yoshihiro4Tao Nariaki5Sagara Kenshi6Department of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityDepartment of Physics, Kyushu UniversityA cross section measurement employing a direct 16O detection method for the reaction energies from Ecm = 2.4 to 0.7 MeV is planned at Kyushu University Tandem Laboratory (KUTL). To perform this experiment and to obtain quantitative information about the cross section to within an error of 10%, we have developed several instruments, including a blow-in type windowless gas target, a recoil mass separator and a RF-deflector. The measurements at Ecm = 2.4 and 1.5 MeV have been performed with these instruments. For measuring at Ecm < 1.2 MeV, a hybrid detector employing both, an ionization chamber and a silicon detector was developed to reduce the carbon backgrounds more efficiently. The oxygen ions were clearly separated from carbon background by using the energy deposit in the ionization chamber. Experiment of Ecm = 1.2 MeV was performed and the cross section was obtained.http://dx.doi.org/10.1051/epjconf/20159303005
collection DOAJ
language English
format Article
sources DOAJ
author Fujita Kunihiro
Yamaguchi Hiroyuki
Ban Tadahiko
Hamamoto Kenichi
Narikiyo Yoshihiro
Tao Nariaki
Sagara Kenshi
spellingShingle Fujita Kunihiro
Yamaguchi Hiroyuki
Ban Tadahiko
Hamamoto Kenichi
Narikiyo Yoshihiro
Tao Nariaki
Sagara Kenshi
Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
EPJ Web of Conferences
author_facet Fujita Kunihiro
Yamaguchi Hiroyuki
Ban Tadahiko
Hamamoto Kenichi
Narikiyo Yoshihiro
Tao Nariaki
Sagara Kenshi
author_sort Fujita Kunihiro
title Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
title_short Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
title_full Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
title_fullStr Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
title_full_unstemmed Direct Measurement of the 4He(12C, 16O)γ Total Cross Section Near Stellar Energies
title_sort direct measurement of the 4he(12c, 16o)γ total cross section near stellar energies
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2015-01-01
description A cross section measurement employing a direct 16O detection method for the reaction energies from Ecm = 2.4 to 0.7 MeV is planned at Kyushu University Tandem Laboratory (KUTL). To perform this experiment and to obtain quantitative information about the cross section to within an error of 10%, we have developed several instruments, including a blow-in type windowless gas target, a recoil mass separator and a RF-deflector. The measurements at Ecm = 2.4 and 1.5 MeV have been performed with these instruments. For measuring at Ecm < 1.2 MeV, a hybrid detector employing both, an ionization chamber and a silicon detector was developed to reduce the carbon backgrounds more efficiently. The oxygen ions were clearly separated from carbon background by using the energy deposit in the ionization chamber. Experiment of Ecm = 1.2 MeV was performed and the cross section was obtained.
url http://dx.doi.org/10.1051/epjconf/20159303005
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