C-12+C-12 fusion in a multichannel folding model
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | |
Tipo de documento: | Artigo de conferência |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNIFESP |
Texto Completo: | http://repositorio.unifesp.br/handle/11600/49662 http://dx.doi.org/10.1088/1742-6596/665/1/012010 |
Resumo: | The C-12+C-12 fusion reaction is investigated using a folding potential in a multichannel approach involving the C-12(0(1)(+),2(+), 0(2)(+), 3(-)) states. The C-12 densities (including transition densities) are taken from the RGM calculation of Kamimura. For the nucleon-nucleon interaction, we use the DDM3Y density-dependent interaction. Owing to the explicit presence of inelastic channels, the imaginary part of the optical potential only contains a short-range fusion contribution. The S-factor is then virtually insensitive to the precise value, and the model is free of any fitting parameter. From the coupled-channel system, we determine the elastic and fusion cross sections simultaneously. As elastic data are available around the Coulomb barrier, this simultaneous treatment offers a good test for the reliability of the model. In the fusion cross section, the role of the inelastic channels and, in particular of the C-12(0(1)(+))+C-12(0(2)(+)) channel involving the Hoyle state, is discussed. |
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Assuncao, M. [UNIFESP]Descouvemont, P.IOP2019-01-21T10:30:16Z2019-01-21T10:30:16Z2016Nuclear Physics In Astrophysics Vi (npa6). Bristol, v. 665, 2016.1742-6588http://repositorio.unifesp.br/handle/11600/49662http://dx.doi.org/10.1088/1742-6596/665/1/01201010.1088/1742-6596/665/1/012010WOS:000368236600010The C-12+C-12 fusion reaction is investigated using a folding potential in a multichannel approach involving the C-12(0(1)(+),2(+), 0(2)(+), 3(-)) states. The C-12 densities (including transition densities) are taken from the RGM calculation of Kamimura. For the nucleon-nucleon interaction, we use the DDM3Y density-dependent interaction. Owing to the explicit presence of inelastic channels, the imaginary part of the optical potential only contains a short-range fusion contribution. The S-factor is then virtually insensitive to the precise value, and the model is free of any fitting parameter. From the coupled-channel system, we determine the elastic and fusion cross sections simultaneously. As elastic data are available around the Coulomb barrier, this simultaneous treatment offers a good test for the reliability of the model. In the fusion cross section, the role of the inelastic channels and, in particular of the C-12(0(1)(+))+C-12(0(2)(+)) channel involving the Hoyle state, is discussed.Univ Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Sao Paulo, BrazilUniv Libre Bruxelles, Phys Nucl Theor & Phys Math, B-1050 Brussels, BelgiumUniv Fed Sao Paulo, Dept Ciencias Exatas & Terra, Campus Diadema, BR-09972270 Sao Paulo, Brazil.Web of ScienceengIop Publishing LtdNuclear Physics In Astrophysics Vi (npa6)Reaction Cross-SectionSubcoulomb EnergiesC-12&C-12C-12ScatteringBarrierC-12+C-12 fusion in a multichannel folding modelinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESP11600/496622021-09-28 16:45:40.702metadata only accessoai:repositorio.unifesp.br:11600/49662Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652021-09-28T19:45:40Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false |
dc.title.en.fl_str_mv |
C-12+C-12 fusion in a multichannel folding model |
title |
C-12+C-12 fusion in a multichannel folding model |
spellingShingle |
C-12+C-12 fusion in a multichannel folding model Assuncao, M. [UNIFESP] Reaction Cross-Section Subcoulomb Energies C-12&C-12 C-12 Scattering Barrier |
title_short |
C-12+C-12 fusion in a multichannel folding model |
title_full |
C-12+C-12 fusion in a multichannel folding model |
title_fullStr |
C-12+C-12 fusion in a multichannel folding model |
title_full_unstemmed |
C-12+C-12 fusion in a multichannel folding model |
title_sort |
C-12+C-12 fusion in a multichannel folding model |
author |
Assuncao, M. [UNIFESP] |
author_facet |
Assuncao, M. [UNIFESP] Descouvemont, P. |
author_role |
author |
author2 |
Descouvemont, P. |
author2_role |
author |
dc.contributor.institution.none.fl_str_mv |
IOP |
dc.contributor.author.fl_str_mv |
Assuncao, M. [UNIFESP] Descouvemont, P. |
dc.subject.eng.fl_str_mv |
Reaction Cross-Section Subcoulomb Energies C-12&C-12 C-12 Scattering Barrier |
topic |
Reaction Cross-Section Subcoulomb Energies C-12&C-12 C-12 Scattering Barrier |
description |
The C-12+C-12 fusion reaction is investigated using a folding potential in a multichannel approach involving the C-12(0(1)(+),2(+), 0(2)(+), 3(-)) states. The C-12 densities (including transition densities) are taken from the RGM calculation of Kamimura. For the nucleon-nucleon interaction, we use the DDM3Y density-dependent interaction. Owing to the explicit presence of inelastic channels, the imaginary part of the optical potential only contains a short-range fusion contribution. The S-factor is then virtually insensitive to the precise value, and the model is free of any fitting parameter. From the coupled-channel system, we determine the elastic and fusion cross sections simultaneously. As elastic data are available around the Coulomb barrier, this simultaneous treatment offers a good test for the reliability of the model. In the fusion cross section, the role of the inelastic channels and, in particular of the C-12(0(1)(+))+C-12(0(2)(+)) channel involving the Hoyle state, is discussed. |
publishDate |
2016 |
dc.date.issued.fl_str_mv |
2016 |
dc.date.accessioned.fl_str_mv |
2019-01-21T10:30:16Z |
dc.date.available.fl_str_mv |
2019-01-21T10:30:16Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.citation.fl_str_mv |
Nuclear Physics In Astrophysics Vi (npa6). Bristol, v. 665, 2016. |
dc.identifier.uri.fl_str_mv |
http://repositorio.unifesp.br/handle/11600/49662 http://dx.doi.org/10.1088/1742-6596/665/1/012010 |
dc.identifier.issn.none.fl_str_mv |
1742-6588 |
dc.identifier.doi.none.fl_str_mv |
10.1088/1742-6596/665/1/012010 |
dc.identifier.wos.none.fl_str_mv |
WOS:000368236600010 |
identifier_str_mv |
Nuclear Physics In Astrophysics Vi (npa6). Bristol, v. 665, 2016. 1742-6588 10.1088/1742-6596/665/1/012010 WOS:000368236600010 |
url |
http://repositorio.unifesp.br/handle/11600/49662 http://dx.doi.org/10.1088/1742-6596/665/1/012010 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
Nuclear Physics In Astrophysics Vi (npa6) |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
Iop Publishing Ltd |
publisher.none.fl_str_mv |
Iop Publishing Ltd |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UNIFESP instname:Universidade Federal de São Paulo (UNIFESP) instacron:UNIFESP |
instname_str |
Universidade Federal de São Paulo (UNIFESP) |
instacron_str |
UNIFESP |
institution |
UNIFESP |
reponame_str |
Repositório Institucional da UNIFESP |
collection |
Repositório Institucional da UNIFESP |
repository.name.fl_str_mv |
Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP) |
repository.mail.fl_str_mv |
|
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1802764153783320576 |