Magnetically charged stars with nonlinear electrodynamics
Khashayar Kianfar

TL;DR
This paper explores magnetically charged stars modeled with nonlinear electrodynamics, revealing an upper mass limit and employing polytropic equations of state to describe these compact objects.
Contribution
It introduces a novel model of magnetically charged stars within a non-singular metric framework using nonlinear electrodynamics, establishing a maximum mass limit.
Findings
Identified an upper mass limit for magnetically charged stars.
Developed a model incorporating nonlinear electrodynamics and polytropic EoS.
Provided insights into the structure of magnetized compact objects.
Abstract
In this research, we introduce magnetically charged stars in the framework of non-singular metric which is explained with nonlinear electrodynamics(NED). This model allows us to have an upper limit for the maximum limit for the mass of stars in the presence of NED. We explain our model for magnetized compact object by considering the polytropic equation of states(EoS)
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Solar and Space Plasma Dynamics
