We determine the complete space-time metric from the bootstrapped Newtonian potential generated by a static spherically symmetric source in the surrounding vacuum. This metric contains post-Newtonian parameters which can be further used to constrain the underlying dynamical theory and quantum state of gravity. For values of the post-Newtonian parameters within experimental bounds, the reconstructed metric appears very close to the Schwarzschild solution of general relativity in the whole region outside the event horizon. The latter is however larger in size for the same value of the mass compared to the Schwarzschild case.

Casadio, R., Giusti, A., Kuntz, I., Neri, G. (2021). Effective metric outside bootstrapped Newtonian sources. PHYSICAL REVIEW D, 103(6), 1-16 [10.1103/PhysRevD.103.064001].

Effective metric outside bootstrapped Newtonian sources

Casadio, Roberto
;
Kuntz, Iberê;Neri, Giulio
2021

Abstract

We determine the complete space-time metric from the bootstrapped Newtonian potential generated by a static spherically symmetric source in the surrounding vacuum. This metric contains post-Newtonian parameters which can be further used to constrain the underlying dynamical theory and quantum state of gravity. For values of the post-Newtonian parameters within experimental bounds, the reconstructed metric appears very close to the Schwarzschild solution of general relativity in the whole region outside the event horizon. The latter is however larger in size for the same value of the mass compared to the Schwarzschild case.
2021
Casadio, R., Giusti, A., Kuntz, I., Neri, G. (2021). Effective metric outside bootstrapped Newtonian sources. PHYSICAL REVIEW D, 103(6), 1-16 [10.1103/PhysRevD.103.064001].
Casadio, Roberto; Giusti, Andrea; Kuntz, Iberê; Neri, Giulio
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/811552
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