Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/341262
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dc.contributor.CRUESPUNIVERSIDADE ESTADUAL DE CAMPINASpt_BR
dc.contributor.authorunicampSouza, Gibran Henrique dept_BR
dc.contributor.authorunicampKemp, Ernestopt_BR
dc.typeArtigopt_BR
dc.titleThe influence of magnetic field geometry in neutron stars' crustal oscillationspt_BR
dc.contributor.authorSouza, G. H. dept_BR
dc.contributor.authorKemp, E.pt_BR
dc.subjectEstrelas de nêutronspt_BR
dc.subjectPulsarespt_BR
dc.subjectNeutron starspt_BR
dc.subjectPulsarspt_BR
dc.description.abstractIn this work, we have studied oscillations in the crust of a neutron star whose magnetic field has both dipolar and toroidal components; the former extends from the stellar interior to the outer space, and the latter is confined inside the star radius. Our study is based on the solutions we have obtained for perturbations in the star fluid, confined to the crust thickness. Our results are compared to the frequencies observed in the soft gamma repeaters signals.pt_BR
dc.relation.ispartofAstronomische nachrichtenpt_BR
dc.relation.ispartofabbreviationAstron. nachr.pt_BR
dc.publisher.cityWeinheimpt_BR
dc.publisher.countryAlemanhapt_BR
dc.publisherWiley-VCH Verlagpt_BR
dc.date.issued2019pt_BR
dc.date.monthofcirculationDec.pt_BR
dc.language.isoengpt_BR
dc.description.firstpagept_BR
dc.description.lastpagept_BR
dc.rightsfechadopt_BR
dc.sourceWOSpt_BR
dc.identifier.issn0004-6337pt_BR
dc.identifier.eissn1521-3994pt_BR
dc.identifier.doi10.1002/asna.201913715pt_BR
dc.identifier.urlhttps://onlinelibrary.wiley.com/doi/full/10.1002/asna.201913715pt_BR
dc.description.sponsorshipFAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsorship1FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsordocumentnumber2014/19164-6pt_BR
dc.date.available2020-05-13T19:34:59Z-
dc.date.accessioned2020-05-13T19:34:59Z-
dc.description.provenanceMade available in DSpace on 2020-05-13T19:34:59Z (GMT). No. of bitstreams: 1 000502794500001.pdf: 1144544 bytes, checksum: 3386bb010518c73e2d2c401efbcb520d (MD5) Previous issue date: 2019en
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/341262-
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.identifier.source000502794500001pt_BR
dc.creator.orcid0000-0001-5835-6737pt_BR
dc.creator.orcid0000-0001-5311-1300pt_BR
dc.type.formArtigopt_BR
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