Description
In this work, we show the solutions of the fluid perturbations equations confined in a neutron star crust with a dipolar magnetic field permeating the whole star. The perturbations are restricted to the crust, and dipolar an toroidal components describe the magnetic field. With this model, we seek to explain the frequencies observed in some Soft Gamma Repeaters flares.
Primary authors
Cecilia Chirenti
Ernesto Kemp
(University of Campinas)
Gibran Henrique de Souza
(University of Campinas - UNICAMP)
