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The Radiant Massive Magnetic Dipole

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arxiv 2310.15979 v1 pith:IXAHQNR2 submitted 2023-10-24 gr-qc math-phmath.MP

José Diaz Polanco , José Ayala , Maximiliano Ujevic This is my paper · ORCID
classification gr-qcmath-phmath.MP
keywords magneticfieldmassivesolutiondipoleeinsteinequationsachieve
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We present an exact, time-dependent solution for the Einstein field equations that models the coupling between an anisotropic fluid and a magnetic field in an axially symmetric space-time. By carefully selecting the metric components, we achieve a convenient separation of variables that enables us to solve Einstein's field equations and obtain a solution that evolves into the Gutsunaev-Manko massive magnetic dipole. The analysis of the thermodynamic quantities suggests that this solution may represent a pulse of radiation emitted by a massive object with magnetic properties as for example pulsars or neutron stars.

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Cited by 1 Pith paper

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  1. Stability of the spacetime of a magnetized compact object

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Scalar perturbations on the exterior of a magnetized Gutsunaev-Manko compact object show quasinormal ringing followed by power-law tails, with stronger magnetization accelerating the ring-down decay.

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