The influence of magnetic field geometry in neutron stars' crustal oscillations

Autor(es)

de Souza, Gibran H. ^[1] ; Kemp, Ernesto ^[1]

Afiliação do(s) autor(es)

^[1] Univ Estadual Campinas UNICAMP, Inst Fis GlebWataghin, BR-13083859 Sao Paulo - Brazil

• Tipo de documento: Artigo Científico
• Fonte: ASTRONOMISCHE NACHRICHTEN; v. 340, n. 9-10, SI, p. 904-908, NOV-DEC 2019.
• Citações Web of Science: 0

Resumo

In 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. (AU)

• Processo FAPESP: 14/19164-6 - Desafios para o século XXI em física e astrofísica de neutrinos
• Beneficiário: Orlando Luis Goulart Peres
• Modalidade de apoio: Auxílio à Pesquisa - Projetos Especiais