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Effective metric outside bootstrapped Newtonian sources

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arxiv 2101.12471 v2 pith:JHGMLFNY submitted 2021-01-29 gr-qc astro-ph.HEhep-th

Roberto Casadio , Andrea Giusti , Iberê Kuntz , Giulio Neri This is my paper · ORCID
classification gr-qcastro-ph.HEhep-th
keywords metricbootstrappedcompletenewtonianoutsideparameterspost-newtonianschwarzschild
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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 complete underlying dynamical theory. 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.

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Cited by 2 Pith papers

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    Gaussian-smearing the gravitational-decoupling hairy black hole produces a regular core and modified photon rings, lensing, and a claimed but absent ringdown spectrum.

  2. Star equilibrium: from BNG to TOV

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Adding TOV-inspired post-Newtonian terms to bootstrapped Newtonian gravity makes the central pressure of homogeneous stars negative before BNG black hole formation, while no Buchdahl limit appears.

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