Black hole binaries in shift-symmetric Einstein-scalar-Gauss-Bonnet gravity experience a slower merger phase
Maxence Corman, Llibert Arest\'e Sal\'o, Katy Clough

TL;DR
This paper investigates how shift-symmetric Einstein-scalar-Gauss-Bonnet gravity alters black hole binary mergers, revealing a transition from faster inspiral due to scalar radiation to a slower late-stage merger caused by non-linear effects.
Contribution
It provides the first non-linear numerical simulations showing the late-stage deceleration of black hole mergers in this modified gravity theory.
Findings
Scalar dipole radiation accelerates early inspiral.
Late-stage merger is decelerated compared to GR.
Non-linear effects significantly alter the merger dynamics.
Abstract
In shift-symmetric Einstein-scalar-Gauss-Bonnet gravity, stationary black holes have a non-vanishing scalar charge. During the inspiral, the phase evolution is modified by several effects, primarily an additional scalar dipole radiation, which enters at -1PN order. This effect accelerates the inspiral when compared to general relativity, when including corrections up to 2PN. Using fully non-linear numerical simulations of quasi-circular, comparable mass binaries, we find that in the late stages the orbital dynamics are altered so that the overall effect is instead a decelerated merger phase for the modified gravity case. We attribute this to a change in the conservative dynamics, and show that at the late inspiral stage more energy must be emitted in scalar-Gauss-Bonnet gravity to induce a given change in frequency. In longer signals, this should lead to a distinctive switch between a…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Black Holes and Theoretical Physics
