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Creators/Authors contains: "Carone, Christopher_D"

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  1. ; (, Classical and Quantum Gravity)
    Abstract Regular black hole metrics involve a universal, mass-independent regulator that can be up to O ( 700 km ) while remaining consistent with terrestrial tests of Newtonian gravity and astrophysical tests of general relativistic orbits. However, for such large values of the regulator scale, the metric describes a compact, astrophysical-mass object with no horizon rather than a black hole. We note that allowing the regulator to have a nontrivial mass dependence preserves the horizon, while allowing large, percent-level effects in black hole observables. By considering the deflection angle of light and the black hole shadow, we demonstrate this possibility explicitly. 
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