Neutron-neutron correlations in light exotic nuclei

Detalhes bibliográficos
Autor(a) principal: Tomio, L. [UNESP]
Data de Publicação: 2005
Outros Autores: Yamashita, Marcelo Takeshi [UNESP], Frederico, T.
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1063/1.1932979
http://hdl.handle.net/11449/68234
Resumo: For light exotic nuclei modeled as two neutrons n and a core A, we report results for the two-neutron correlation functions and also for the mean-square radii, considering a universal scaling function. The results of our calculations for the neutron-neutron correlation functions are qualitatively consistent with recent data obtained for 11Li and 14Be nuclei. The root-mean-square distance in the halo of such nuclei are also consistent with data, which means that the neutrons of the halo have a large probability to be found outside the interaction range. Therefore the low-energy properties of these halo neutrons are, to a large extend, model independent as long as few physical input scales are fixed. The model is restricted to s-wave subsystems, with small energies for the bound or virtual states. For the radii we are also shown results for the 6He and 20C. All the interaction effects, as higher partial wave in the interaction and/or Pauli blocking effect are, to some extend, included in our model, as long as the three-body binding energy is supplied. © 2005 American Institute of Physics.
id UNSP_1fe77438bfeaaf8b41a2e77e3689afb7
oai_identifier_str oai:repositorio.unesp.br:11449/68234
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling Neutron-neutron correlations in light exotic nucleiFor light exotic nuclei modeled as two neutrons n and a core A, we report results for the two-neutron correlation functions and also for the mean-square radii, considering a universal scaling function. The results of our calculations for the neutron-neutron correlation functions are qualitatively consistent with recent data obtained for 11Li and 14Be nuclei. The root-mean-square distance in the halo of such nuclei are also consistent with data, which means that the neutrons of the halo have a large probability to be found outside the interaction range. Therefore the low-energy properties of these halo neutrons are, to a large extend, model independent as long as few physical input scales are fixed. The model is restricted to s-wave subsystems, with small energies for the bound or virtual states. For the radii we are also shown results for the 6He and 20C. All the interaction effects, as higher partial wave in the interaction and/or Pauli blocking effect are, to some extend, included in our model, as long as the three-body binding energy is supplied. © 2005 American Institute of Physics.Instituto de Física Teórica UNESP, 01405-900, São Paulo, SPLaboratório Do Acelerador Linear Instituto de Física Universidade de São Paulo, CEP, 05315-970, São PauloDep. de Física Instituto Tecnológico de Aeronáutica Centro Técnico Aeroespacial, 12228-900, Sao Jose dos CamposInstituto de Física Teórica UNESP, 01405-900, São Paulo, SPUniversidade Estadual Paulista (Unesp)Universidade de São Paulo (USP)Centro Técnico AeroespacialTomio, L. [UNESP]Yamashita, Marcelo Takeshi [UNESP]Frederico, T.2014-05-27T11:21:20Z2014-05-27T11:21:20Z2005-05-06info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject401-403application/pdfhttp://dx.doi.org/10.1063/1.1932979AIP Conference Proceedings, v. 768, p. 401-403.0094-243X1551-7616http://hdl.handle.net/11449/6823410.1063/1.1932979WOS:0002297804001192-s2.0-337493774722-s2.0-33749377472.pdf3740639726545315Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAIP Conference Proceedingsinfo:eu-repo/semantics/openAccess2023-11-02T06:10:03Zoai:repositorio.unesp.br:11449/68234Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-11-02T06:10:03Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Neutron-neutron correlations in light exotic nuclei
title Neutron-neutron correlations in light exotic nuclei
spellingShingle Neutron-neutron correlations in light exotic nuclei
Tomio, L. [UNESP]
title_short Neutron-neutron correlations in light exotic nuclei
title_full Neutron-neutron correlations in light exotic nuclei
title_fullStr Neutron-neutron correlations in light exotic nuclei
title_full_unstemmed Neutron-neutron correlations in light exotic nuclei
title_sort Neutron-neutron correlations in light exotic nuclei
author Tomio, L. [UNESP]
author_facet Tomio, L. [UNESP]
Yamashita, Marcelo Takeshi [UNESP]
Frederico, T.
author_role author
author2 Yamashita, Marcelo Takeshi [UNESP]
Frederico, T.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Universidade de São Paulo (USP)
Centro Técnico Aeroespacial
dc.contributor.author.fl_str_mv Tomio, L. [UNESP]
Yamashita, Marcelo Takeshi [UNESP]
Frederico, T.
description For light exotic nuclei modeled as two neutrons n and a core A, we report results for the two-neutron correlation functions and also for the mean-square radii, considering a universal scaling function. The results of our calculations for the neutron-neutron correlation functions are qualitatively consistent with recent data obtained for 11Li and 14Be nuclei. The root-mean-square distance in the halo of such nuclei are also consistent with data, which means that the neutrons of the halo have a large probability to be found outside the interaction range. Therefore the low-energy properties of these halo neutrons are, to a large extend, model independent as long as few physical input scales are fixed. The model is restricted to s-wave subsystems, with small energies for the bound or virtual states. For the radii we are also shown results for the 6He and 20C. All the interaction effects, as higher partial wave in the interaction and/or Pauli blocking effect are, to some extend, included in our model, as long as the three-body binding energy is supplied. © 2005 American Institute of Physics.
publishDate 2005
dc.date.none.fl_str_mv 2005-05-06
2014-05-27T11:21:20Z
2014-05-27T11:21:20Z
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/10.1063/1.1932979
AIP Conference Proceedings, v. 768, p. 401-403.
0094-243X
1551-7616
http://hdl.handle.net/11449/68234
10.1063/1.1932979
WOS:000229780400119
2-s2.0-33749377472
2-s2.0-33749377472.pdf
3740639726545315
url http://dx.doi.org/10.1063/1.1932979
http://hdl.handle.net/11449/68234
identifier_str_mv AIP Conference Proceedings, v. 768, p. 401-403.
0094-243X
1551-7616
10.1063/1.1932979
WOS:000229780400119
2-s2.0-33749377472
2-s2.0-33749377472.pdf
3740639726545315
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv AIP Conference Proceedings
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 401-403
application/pdf
dc.source.none.fl_str_mv Scopus
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_ 1803046284041388032