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arXiv · 2205.07088

Planck Stars from a Scale-dependent Gravity theory

Fabio Scardigli·Gaetano Lambiase
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Abstract

Scale dependence of fundamental physical parameters is a generic feature of ordinary quantum field theory. When applied to gravity, this idea produces effective actions generically containing a running Newtonian coupling constant, from which new (spherically symmetric) black hole spacetimes can be inferred. As a minimum useful requirement, of course, the new metrics should match with a Schwarzschild field at large radial coordinate. By further imposing to the new scale dependent metric the simple request of matching with the Donoghue quantum corrected potential, we find a not yet explored black hole spacetime, which naturally turns out to describe the so-called Planck stars.

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Fabio Scardigli, Gaetano Lambiase. 2022-05-14. Planck Stars from a Scale-dependent Gravity theory. https://doi.org/10.1103/physrevd.107.104001

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