Speaker
Daryel Manreza Paret
(Department of General Physics, Faculty of Physics, University of Havana)
Description
We study the effects of magnetic fields on gravitational wave signals emitted from isolated quark stars due to deformation caused by the strong magnetic field. For this purpose we construct a toy model in order to make estimates of the order of magnitude of the magnetic field that will cause sufficient deformation in a quark star for the detection of gravitational waves.
Authors
Daryel Manreza Paret
(Department of General Physics, Faculty of Physics, University of Havana)
Samantha López Pérez
(Department of Theoretical Physics, Institute of Cybernetics, Mathematics and Physics)
Aurora Pérez Martínez
(Department of Theoretical Physics, Institute of Cybernetics, Mathematics and Physics)
