dor_id: 4108087

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650.#.4.x: Físico Matemáticas y Ciencias de la Tierra

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856.4.0.u: https://rmf.smf.mx/ojs/rmf/article/view/Vol.%2065%2C%20Issue%202%2C%20pp.%20159-167/4241; https://rmf.smf.mx/ojs/rmf/article/downloadSuppFile/Vol.%2065%2C%20Issue%202%2C%20pp.%20159-167/423

100.1.#.a: Majeed, Fouad A.; Obaid, Sarah M.

524.#.#.a: Majeed, Fouad A., et al. (2019). Nuclear structure study of [22,24]Ne and [24]Mg nuclei. Revista Mexicana de Física; Vol 65, No 2 Mar-Apr: 159-167. Recuperado de https://repositorio.unam.mx/contenidos/4108087

245.1.0.a: Nuclear structure study of [22,24]Ne and [24]Mg nuclei

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Facultad de Ciencias, UNAM

264.#.0.c: 2019

264.#.1.c: 2019-03-26

653.#.#.a: Nuclear structure, electron scattering form factors, core polarization effects

506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC-ND 4.0 Internacional, https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.es, fecha de asignación de la licencia 2019-03-26, para un uso diferente consultar al responsable jurídico del repositorio por medio de rmf@ciencias.unam.mx

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001.#.#.#: oai:ojs.rmf.smf.mx:article/479

041.#.7.h: eng

520.3.#.a: Shell model calculations based on large basis has been conducted to study the nuclear structure of 20 Ne, 22 Ne and 24 Mg nuclei. The energy levels, inelastic electron scattering form factors and transition probabilities are discussed by considering the contribution of  configurations with high-energy beyond the model space of sd-shell model space which is denoted as the core polarization (CP) effects.simThe Core polarization is considered by taking the excitations of nucleus from the 1s and 1p core orbits and also from the valence 2s 1d shell orbit in to higher shells with 4\hbar\ω. The effective interactions USDA and USDB are employed with sd shell model space to perform the calculation and the core polarization are calculated with MSDI as residual interaction.simThe calculated energy level schemes,  form factors and transition probabilities were compared with the corresponding experimental data. The effect of core polarization is found very important for the calculation of B(C2), B(C4) and form factors, and gives excellent results in comparison with the experimental data without including any adjustable parameters.

773.1.#.t: Revista Mexicana de Física; Vol 65, No 2 Mar-Apr (2019): 159-167

773.1.#.o: https://rmf.smf.mx/ojs/rmf/index

046.#.#.j: 2020-11-25 00:00:00.000000

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doi: https://doi.org/10.31349/RevMexFis.65.159

handle: 00ed628089295652

harvesting_date: 2020-09-23 00:00:00.0

856.#.0.q: application/pdf

last_modified: 2020-11-27 00:00:00

license_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.es

license_type: by-nc-nd

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Artículo

Nuclear structure study of [22,24]Ne and [24]Mg nuclei

Majeed, Fouad A.; Obaid, Sarah M.

Facultad de Ciencias, UNAM, publicado en Revista Mexicana de Física, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Entidad o dependencia
Facultad de Ciencias, UNAM
Revista
Repositorio
Contacto
Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

Cita

Majeed, Fouad A., et al. (2019). Nuclear structure study of [22,24]Ne and [24]Mg nuclei. Revista Mexicana de Física; Vol 65, No 2 Mar-Apr: 159-167. Recuperado de https://repositorio.unam.mx/contenidos/4108087

Descripción del recurso

Autor(es)
Majeed, Fouad A.; Obaid, Sarah M.
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
Nuclear structure study of [22,24]Ne and [24]Mg nuclei
Fecha
2019-03-26
Resumen
Shell model calculations based on large basis has been conducted to study the nuclear structure of 20 Ne, 22 Ne and 24 Mg nuclei. The energy levels, inelastic electron scattering form factors and transition probabilities are discussed by considering the contribution of  configurations with high-energy beyond the model space of sd-shell model space which is denoted as the core polarization (CP) effects.simThe Core polarization is considered by taking the excitations of nucleus from the 1s and 1p core orbits and also from the valence 2s 1d shell orbit in to higher shells with 4\hbar\ω. The effective interactions USDA and USDB are employed with sd shell model space to perform the calculation and the core polarization are calculated with MSDI as residual interaction.simThe calculated energy level schemes,  form factors and transition probabilities were compared with the corresponding experimental data. The effect of core polarization is found very important for the calculation of B(C2), B(C4) and form factors, and gives excellent results in comparison with the experimental data without including any adjustable parameters.
Tema
Nuclear structure, electron scattering form factors, core polarization effects
Idioma
eng
ISSN
2683-2224 (digital); 0035-001X (impresa)

Enlaces