21-27 October 2018
Hermosillo, Sonora
MST timezone
- jose.benitez@cern.ch
Support
Contribution
Speakers
- Prof. Aurora PEREZ MARTINEZ
Primary authors
- Prof. Aurora PEREZ MARTINEZ (Instituto de Cibernetica Matematica y Fisica (ICIMAF))
Co-authors
- Diana ALVEAR TERRERO (Instituto de Cibernetica Matematica y Fisica)
- Gretel QUINTERO ANGULO (Facultad de Fisica, Universidad de la Habana)
- Daryel MANREZA PARET (Facultad de Fisica Universidad de la Habana)
- Samantha LOPEZ PEREZ (Instituto de Cibernetica Matematica y Fisica)
- Prof. Victoria HERMANDEZ MEDEROS (Instituto de Cibernetica Matematica y Fisica)
Content
Magnetic fields are present in compact objects affecting its structure. The anisotropy produced by the magnetic field in the pressures suggests the necessity of using structure equations considering the axial symmetry of the magnetized system. In this work, we propose a model that generalizes the Tolman-Oppenheimer-Volkoff equations for the magnetized case and discuss some preliminary results. Our calculations are based on the \gamma-metrics where the parameter \gamma relates the deformation with the anisotropy in the pressures.
Category
Theory/Pheno