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Schwarzschild metric from Scattering Amplitudes to all orders in $G_N$

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arxiv 2405.14421 v2 pith:CKMTT4BP submitted 2024-05-23 hep-th gr-qc

classification hep-thgr-qc
keywords metricordersschwarzschildblackcubicformulationholeinteractions
verification ladder T0 review T1 audit T2 compute T3 formal
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We apply a formulation of Einstein's general relativity with only cubic interactions for deriving the metric of a Schwarzschild black hole to all orders in perturbation theory. This cubic interactions formulation coupled to effective worldline action of a massive point particle allows to derive a recursion relation for the form factors of the off-shell graviton emission current. The unique solution to the recursion relation leads to the Schwarzschild black-hole solution in four dimensions. This provides the first derivation of the black hole metric from a matter source to all orders in perturbation theory from an amplitude approach.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Radiation-Reaction and Angular Momentum Loss at $\mathcal{O}(G^4)$

    hep-th 2025-01 accept novelty 8.0 of 10

    A closed-form, all-velocity expression for the O(G^4) radiated angular momentum in two-body gravitational scattering is derived, resumming all half-odd post-Newtonian corrections.

  2. Generalized Wilson lines and the gravitational scattering of spinning bodies

    hep-th 2024-12 conditional novelty 7.0 of 10

    A new generalized Wilson line representation for spin-1/2 and classical spinning bodies is derived, reproducing known 2PM gravitational scattering observables.

  3. One loop analysis of the cubic action for gravity

    hep-th 2025-02 conditional novelty 6.0 of 10

    The cubic Palatini gravity action is BRST-consistent at one loop around flat space only after finite counterterms beyond minimal subtraction are added.

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