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The 14C(n,γ) cross section between 10 keV and 1 M

The neutron capture cross section of 14C is of relevance for several nucleosynthesis scenarios such as inhomogeneous Big Bang models, neutron induced CNO cycles, and neutrino driven wind models for the r process. The 14C(n,γ) reaction is also important for the validation of the Coulomb dissociation...

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Detalles Bibliográficos
Autores principales: Reifarth, R, Heil, M, Forssén, C, Besserer, U, Couture, A, Dababneh, S, Dörr, L, Görres, J, Haight, R C, Käppeler, F, Mengoni, A, O'Brien, S, Patronis, N, Plag, R, Rundberg, R S, Wiescher, M, Wilhelmy, J B
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevC.77.015804
http://cds.cern.ch/record/1210293
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author Reifarth, R
Heil, M
Forssén, C
Besserer, U
Couture, A
Dababneh, S
Dörr, L
Görres, J
Haight, R C
Käppeler, F
Mengoni, A
O'Brien, S
Patronis, N
Plag, R
Rundberg, R S
Wiescher, M
Wilhelmy, J B
author_facet Reifarth, R
Heil, M
Forssén, C
Besserer, U
Couture, A
Dababneh, S
Dörr, L
Görres, J
Haight, R C
Käppeler, F
Mengoni, A
O'Brien, S
Patronis, N
Plag, R
Rundberg, R S
Wiescher, M
Wilhelmy, J B
author_sort Reifarth, R
collection CERN
description The neutron capture cross section of 14C is of relevance for several nucleosynthesis scenarios such as inhomogeneous Big Bang models, neutron induced CNO cycles, and neutrino driven wind models for the r process. The 14C(n,γ) reaction is also important for the validation of the Coulomb dissociation method, where the (n,γ) cross section can be indirectly obtained via the time-reversed process. So far, the example of 14C is the only case with neutrons where both, direct measurement and indirect Coulomb dissociation, have been applied. Unfortunately, the interpretation is obscured by discrepancies between several experiments and theory. Therefore, we report on new direct measurements of the 14C(n,γ) reaction with neutron energies ranging from 20 to 800 keV.
id cern-1210293
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
record_format invenio
spelling cern-12102932019-09-30T06:29:59Zdoi:10.1103/PhysRevC.77.015804http://cds.cern.ch/record/1210293engReifarth, RHeil, MForssén, CBesserer, UCouture, ADababneh, SDörr, LGörres, JHaight, R CKäppeler, FMengoni, AO'Brien, SPatronis, NPlag, RRundberg, R SWiescher, MWilhelmy, J BThe 14C(n,γ) cross section between 10 keV and 1 Mastro-ph.IMThe neutron capture cross section of 14C is of relevance for several nucleosynthesis scenarios such as inhomogeneous Big Bang models, neutron induced CNO cycles, and neutrino driven wind models for the r process. The 14C(n,γ) reaction is also important for the validation of the Coulomb dissociation method, where the (n,γ) cross section can be indirectly obtained via the time-reversed process. So far, the example of 14C is the only case with neutrons where both, direct measurement and indirect Coulomb dissociation, have been applied. Unfortunately, the interpretation is obscured by discrepancies between several experiments and theory. Therefore, we report on new direct measurements of the 14C(n,γ) reaction with neutron energies ranging from 20 to 800 keV.arXiv:0910.0106APS-123-QEDoai:cds.cern.ch:12102932009-10-02
spellingShingle astro-ph.IM
Reifarth, R
Heil, M
Forssén, C
Besserer, U
Couture, A
Dababneh, S
Dörr, L
Görres, J
Haight, R C
Käppeler, F
Mengoni, A
O'Brien, S
Patronis, N
Plag, R
Rundberg, R S
Wiescher, M
Wilhelmy, J B
The 14C(n,γ) cross section between 10 keV and 1 M
title The 14C(n,γ) cross section between 10 keV and 1 M
title_full The 14C(n,γ) cross section between 10 keV and 1 M
title_fullStr The 14C(n,γ) cross section between 10 keV and 1 M
title_full_unstemmed The 14C(n,γ) cross section between 10 keV and 1 M
title_short The 14C(n,γ) cross section between 10 keV and 1 M
title_sort 14c(n,γ) cross section between 10 kev and 1 m
topic astro-ph.IM
url https://dx.doi.org/10.1103/PhysRevC.77.015804
http://cds.cern.ch/record/1210293
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