| Full text | |
| Author(s): |
Total Authors: 2
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| Affiliation: | [1] Univ Estadual Campinas UNICAMP, Inst Fis GlebWataghin, BR-13083859 Sao Paulo - Brazil
Total Affiliations: 1
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| Document type: | Journal article |
| Source: | ASTRONOMISCHE NACHRICHTEN; v. 340, n. 9-10, SI, p. 904-908, NOV-DEC 2019. |
| Web of Science Citations: | 0 |
| Abstract | |
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) | |
| FAPESP's process: | 14/19164-6 - Challenges in the 21st century in neutrino physics and astrophysics |
| Grantee: | Orlando Luis Goulart Peres |
| Support Opportunities: | Special Projects |