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.File | Dimensione | Formato | |
---|---|---|---|
BootEffectiveMetric_arXivV2.pdf
accesso aperto
Tipo:
Postprint
Licenza:
Licenza per accesso libero gratuito
Dimensione
716.1 kB
Formato
Adobe PDF
|
716.1 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.