Nuclear masses, deformations and shell effects
- Autores
- Hirsch, Jorge Gustavo; Barbero, César Alberto; Mariano, Alejandro Edgardo
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We show that the Liquid Drop Model is best suited to describe the masses of prolate deformed nuclei than of spherical nuclei. To this end three Liquid Drop Mass formulas are employed to describe nuclear masses of eight sets of nuclei with similar quadrupole deformations. It is shown that they are able to fit the measured masses of prolate deformed nuclei with an RMS smaller than 750 keV, while for the spherical nuclei the RMS is, in the three cases, larger than 2000 keV. The RMS of the best fit of the masses of semi-magic nuclei is also larger than 2000 keV. The parameters of the three models are studied, showing that the surface symmetry term is the one which varies the most from one group of nuclei to another. In one model, isospin dependent terms are also found to exhibit strong changes. The inclusion of shell effects allows for better fits, which continue to be better in the prolate deformed nuclei region.
Facultad de Ciencias Exactas - Materia
-
Ciencias Exactas
Física
Liquid Drop Model
Nuclear masses
symmetry - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/128639
Ver los metadatos del registro completo
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Nuclear masses, deformations and shell effectsHirsch, Jorge GustavoBarbero, César AlbertoMariano, Alejandro EdgardoCiencias ExactasFísicaLiquid Drop ModelNuclear massessymmetryWe show that the Liquid Drop Model is best suited to describe the masses of prolate deformed nuclei than of spherical nuclei. To this end three Liquid Drop Mass formulas are employed to describe nuclear masses of eight sets of nuclei with similar quadrupole deformations. It is shown that they are able to fit the measured masses of prolate deformed nuclei with an RMS smaller than 750 keV, while for the spherical nuclei the RMS is, in the three cases, larger than 2000 keV. The RMS of the best fit of the masses of semi-magic nuclei is also larger than 2000 keV. The parameters of the three models are studied, showing that the surface symmetry term is the one which varies the most from one group of nuclei to another. In one model, isospin dependent terms are also found to exhibit strong changes. The inclusion of shell effects allows for better fits, which continue to be better in the prolate deformed nuclei region.Facultad de Ciencias Exactas2011-10-31info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/128639enginfo:eu-repo/semantics/altIdentifier/issn/1742-6596info:eu-repo/semantics/altIdentifier/arxiv/1108.0707info:eu-repo/semantics/altIdentifier/doi/10.1088/1742-6596/322/1/012017info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:22:50Zoai:sedici.unlp.edu.ar:10915/128639Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:22:50.288SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Nuclear masses, deformations and shell effects |
title |
Nuclear masses, deformations and shell effects |
spellingShingle |
Nuclear masses, deformations and shell effects Hirsch, Jorge Gustavo Ciencias Exactas Física Liquid Drop Model Nuclear masses symmetry |
title_short |
Nuclear masses, deformations and shell effects |
title_full |
Nuclear masses, deformations and shell effects |
title_fullStr |
Nuclear masses, deformations and shell effects |
title_full_unstemmed |
Nuclear masses, deformations and shell effects |
title_sort |
Nuclear masses, deformations and shell effects |
dc.creator.none.fl_str_mv |
Hirsch, Jorge Gustavo Barbero, César Alberto Mariano, Alejandro Edgardo |
author |
Hirsch, Jorge Gustavo |
author_facet |
Hirsch, Jorge Gustavo Barbero, César Alberto Mariano, Alejandro Edgardo |
author_role |
author |
author2 |
Barbero, César Alberto Mariano, Alejandro Edgardo |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Exactas Física Liquid Drop Model Nuclear masses symmetry |
topic |
Ciencias Exactas Física Liquid Drop Model Nuclear masses symmetry |
dc.description.none.fl_txt_mv |
We show that the Liquid Drop Model is best suited to describe the masses of prolate deformed nuclei than of spherical nuclei. To this end three Liquid Drop Mass formulas are employed to describe nuclear masses of eight sets of nuclei with similar quadrupole deformations. It is shown that they are able to fit the measured masses of prolate deformed nuclei with an RMS smaller than 750 keV, while for the spherical nuclei the RMS is, in the three cases, larger than 2000 keV. The RMS of the best fit of the masses of semi-magic nuclei is also larger than 2000 keV. The parameters of the three models are studied, showing that the surface symmetry term is the one which varies the most from one group of nuclei to another. In one model, isospin dependent terms are also found to exhibit strong changes. The inclusion of shell effects allows for better fits, which continue to be better in the prolate deformed nuclei region. Facultad de Ciencias Exactas |
description |
We show that the Liquid Drop Model is best suited to describe the masses of prolate deformed nuclei than of spherical nuclei. To this end three Liquid Drop Mass formulas are employed to describe nuclear masses of eight sets of nuclei with similar quadrupole deformations. It is shown that they are able to fit the measured masses of prolate deformed nuclei with an RMS smaller than 750 keV, while for the spherical nuclei the RMS is, in the three cases, larger than 2000 keV. The RMS of the best fit of the masses of semi-magic nuclei is also larger than 2000 keV. The parameters of the three models are studied, showing that the surface symmetry term is the one which varies the most from one group of nuclei to another. In one model, isospin dependent terms are also found to exhibit strong changes. The inclusion of shell effects allows for better fits, which continue to be better in the prolate deformed nuclei region. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-10-31 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/128639 |
url |
http://sedici.unlp.edu.ar/handle/10915/128639 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1742-6596 info:eu-repo/semantics/altIdentifier/arxiv/1108.0707 info:eu-repo/semantics/altIdentifier/doi/10.1088/1742-6596/322/1/012017 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf |
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