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Scattering of massless scalar field by charged dilatonic black holes

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arxiv 2006.01388 v2 pith:OU4SUSC7 submitted 2020-06-02 gr-qc

classification gr-qc
keywords blackscatteringwaveholescalarcrossdilatonicfield
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Wave propagations in the presence of black holes is a significant problem both in theoretical and observational aspects, especially after the discovery of gravitational wave and confirmation of black holes. We study the scattering of massless scalar field by a charged dilatonic black hole in frame of full wave theory. We apply partial wave method to obtain the scattering cross sections of the scalar field, and investigate how the black hole charge affects the scalar scattering cross sections. Furthermore, we investigate the Regge pole approach of the scattering cross section of the dilatonic black hole. We find that in order to obtain results at the same precision, we need more Regge poles as the black hole charge increases. We compare the results in the full wave theory and results in the classical geodesic scattering and the semi-classical glory approximations, and demonstrate the improvements and power of our approach.

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Cited by 2 Pith papers

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

  1. Spin precession in the strong deflection limit

    gr-qc 2026-07 conditional novelty 6.0 of 10

    Spin precession near black holes diverges logarithmically in the strong-deflection limit and is related to the deflection angle by a compact formula.

  2. Stability Analysis of Circular Geodesics in Dyonic Dilatonic Black Hole Spacetimes

    gr-qc 2024-11 conditional novelty 4.0 of 10

    A proof that dyonic-like dilatonic black holes have a unique innermost stable circular orbit, plus explicit ISCO formulas for selected values of the dilaton coupling parameter.

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