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Time dependent black holes and gravitational wave in Einstein-Gauss-Bonnet theory with two scalar fields

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arxiv 2411.02439 v1 pith:AERAVQ7Q submitted 2024-11-02 gr-qc hep-th

Time dependent black holes and gravitational wave in Einstein-Gauss-Bonnet theory with two scalar fields

classification gr-qc hep-th
keywords blackgravitationalholeswavescouplingeinstein-gauss-bonnetexaminingfields
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper explores time-varying black holes within the framework of the Einstein-Gauss-Bonnet theory with two scalar fields, examining the propagation of gravitational waves (GW). In reconstructed models, ghosts frequently emerge but can be eliminated by applying certain constraints. We investigate the behavior of high-frequency gravitational waves by examining the effects of varying Gauss-Bonnet coupling during their propagation. The speed of transmission is altered by the coupling in the creation of black holes. The speed of gravitational waves varies as they enter a black hole compared to when they exit.

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Cited by 1 Pith paper

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  1. Beyond general relativity: gravitational waves in non-minimally coupled theories

    gr-qc 2025-10 conditional novelty 5.0

    A generalized propagation parameterization for gravitational-wave strains is extended to O(H²) and O(H′), then mapped to Kalb-Ramond, axion-dilaton–Chern-Simons–Gauss-Bonnet, and U(1) dark-photon models.