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Analytical representation for metrics of scalarized Einstein-Maxwell black holes and their shadows
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Here we construct approximate analytical forms for the metric coefficients and fields representing the scalarized Einstein-Maxwell black holes with various couplings of the scalar field, once the parameters of the system are fixed. By increasing approximation order, one can obtain the analytic representation with any desired accuracy, what was tested via calculations of shadows for these black holes by using approximate analytical and accurate numerical metric functions. We share the Mathematica code which allows one to find an appropriate analytical form of the metric for any couplings and values of parameters. Scalarization increases the radius of the black-hole shadow for all the considered coupling functions.
Forward citations
Cited by 2 Pith papers
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On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows
The authors introduce two new regular black hole metrics from nonlinear electrodynamics and two Limiting Curvature Condition versions, with numerical results for stability, shadows, and quasinormal modes.
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Analytically approximated scalarized black holes and their thermodynamic stability
Scalarized black holes in quadratic Einstein-scalar-Gauss-Bonnet gravity have lower horizon entropy than Schwarzschild, so they may decay back to Schwarzschild.
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