3D calculation of Tucson-Melbourne 3NF effect in triton binding energy
Autor(a) principal: | |
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Data de Publicação: | 2010 |
Outros Autores: | , |
Tipo de documento: | Artigo de conferência |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1063/1.3480267 http://hdl.handle.net/11449/24359 |
Resumo: | As an application of the new realistic three-dimensional (3D) formalism reported recently for three-nucleon (3N) bound states, an attempt is made to study the effect of three-nucleon forces (3NFs) in triton binding energy in a non partial wave (PW) approach. The spin-isospin dependent 3N Faddeev integral equations with the inclusion of 3NFs, which are formulated as function of vector Jacobi momenta, specifically the magnitudes of the momenta and the angle between them, are solved with Bonn-B and Tucson-Melbourne NN and 3N forces in operator forms which can be incorporated in our 3D formalism. The comparison with numerical results in both, novel 3D and standard PW schemes, shows that non PW calculations avoid the very involved angular momentum algebra occurring for the permutations and transformations and it is more efficient and less cumbersome for considering the 3NF. |
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Repositório Institucional da UNESP |
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3D calculation of Tucson-Melbourne 3NF effect in triton binding energytriton binding energythree dimensional approachBonn-BTucson-Melbournethree-nucleon forceAs an application of the new realistic three-dimensional (3D) formalism reported recently for three-nucleon (3N) bound states, an attempt is made to study the effect of three-nucleon forces (3NFs) in triton binding energy in a non partial wave (PW) approach. The spin-isospin dependent 3N Faddeev integral equations with the inclusion of 3NFs, which are formulated as function of vector Jacobi momenta, specifically the magnitudes of the momenta and the angle between them, are solved with Bonn-B and Tucson-Melbourne NN and 3N forces in operator forms which can be incorporated in our 3D formalism. The comparison with numerical results in both, novel 3D and standard PW schemes, shows that non PW calculations avoid the very involved angular momentum algebra occurring for the permutations and transformations and it is more efficient and less cumbersome for considering the 3NF.Univ Estadual Paulista UNESP, IFT, BR-01140070 São Paulo, BrazilUniv Estadual Paulista UNESP, IFT, BR-01140070 São Paulo, BrazilAmerican Institute of Physics (AIP)Universidade Estadual Paulista (Unesp)Hadizadeh, M. R. [UNESP]Tomio, L. [UNESP]Bayegan, S.2013-09-30T18:56:18Z2014-05-20T14:10:45Z2013-09-30T18:56:18Z2014-05-20T14:10:45Z2010-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject84-87application/pdfhttp://dx.doi.org/10.1063/1.3480267Viii Latin American Symposium on Nuclear Physics and Applications. Melville: Amer Inst Physics, v. 1265, p. 84-87, 2010.0094-243Xhttp://hdl.handle.net/11449/2435910.1063/1.3480267WOS:0002871648000172-s2.0-786499337182-s2.0-78649933718.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengViii Latin American Symposium on Nuclear Physics and Applicationsinfo:eu-repo/semantics/openAccess2023-11-17T06:08:48Zoai:repositorio.unesp.br:11449/24359Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:53:57.598584Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
title |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
spellingShingle |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy Hadizadeh, M. R. [UNESP] triton binding energy three dimensional approach Bonn-B Tucson-Melbourne three-nucleon force |
title_short |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
title_full |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
title_fullStr |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
title_full_unstemmed |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
title_sort |
3D calculation of Tucson-Melbourne 3NF effect in triton binding energy |
author |
Hadizadeh, M. R. [UNESP] |
author_facet |
Hadizadeh, M. R. [UNESP] Tomio, L. [UNESP] Bayegan, S. |
author_role |
author |
author2 |
Tomio, L. [UNESP] Bayegan, S. |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Hadizadeh, M. R. [UNESP] Tomio, L. [UNESP] Bayegan, S. |
dc.subject.por.fl_str_mv |
triton binding energy three dimensional approach Bonn-B Tucson-Melbourne three-nucleon force |
topic |
triton binding energy three dimensional approach Bonn-B Tucson-Melbourne three-nucleon force |
description |
As an application of the new realistic three-dimensional (3D) formalism reported recently for three-nucleon (3N) bound states, an attempt is made to study the effect of three-nucleon forces (3NFs) in triton binding energy in a non partial wave (PW) approach. The spin-isospin dependent 3N Faddeev integral equations with the inclusion of 3NFs, which are formulated as function of vector Jacobi momenta, specifically the magnitudes of the momenta and the angle between them, are solved with Bonn-B and Tucson-Melbourne NN and 3N forces in operator forms which can be incorporated in our 3D formalism. The comparison with numerical results in both, novel 3D and standard PW schemes, shows that non PW calculations avoid the very involved angular momentum algebra occurring for the permutations and transformations and it is more efficient and less cumbersome for considering the 3NF. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-01-01 2013-09-30T18:56:18Z 2013-09-30T18:56:18Z 2014-05-20T14:10:45Z 2014-05-20T14:10:45Z |
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.uri.fl_str_mv |
http://dx.doi.org/10.1063/1.3480267 Viii Latin American Symposium on Nuclear Physics and Applications. Melville: Amer Inst Physics, v. 1265, p. 84-87, 2010. 0094-243X http://hdl.handle.net/11449/24359 10.1063/1.3480267 WOS:000287164800017 2-s2.0-78649933718 2-s2.0-78649933718.pdf |
url |
http://dx.doi.org/10.1063/1.3480267 http://hdl.handle.net/11449/24359 |
identifier_str_mv |
Viii Latin American Symposium on Nuclear Physics and Applications. Melville: Amer Inst Physics, v. 1265, p. 84-87, 2010. 0094-243X 10.1063/1.3480267 WOS:000287164800017 2-s2.0-78649933718 2-s2.0-78649933718.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Viii Latin American Symposium on Nuclear Physics and Applications |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
84-87 application/pdf |
dc.publisher.none.fl_str_mv |
American Institute of Physics (AIP) |
publisher.none.fl_str_mv |
American Institute of Physics (AIP) |
dc.source.none.fl_str_mv |
Web of Science reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808128226430550016 |