2019/05/31 by Leong Khim Wong
Physics and Astronomy · #Astrophysical Phenomena and Observations #Binary black hole #Binary number #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Computation #Computer science #Gravitational wave #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Scalar (mathematics) #Scalar field #Superradiance #Theoretical physics #astro-ph.HE #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.100.044051
published as Phys. Rev. D 100, 044051 (2019) · Version accepted for publication. 5 pages. A few extra details added, technical details moved to an appendix
arxiv created 2019/08/24 · openalex publication_date 2019/08/28 · arxiv updated 2019/09/02 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
I present evidence of a novel guise of superradiance that arises in black hole binary spacetimes. Given the right initial conditions, a wave will be amplified as it scatters off the binary. This process, which extracts energy from the orbital motion, is driven by absorption across the horizons and is most pronounced when the individual black holes are not spinning. Focusing on real scalar fields, I demonstrate how modern effective field theory (EFT) techniques enable the computation of the superradiant amplification factor analytically when there exist large separations of scales. Although exploiting these hierarchies inevitably means that the amplification factor is always negligible (it is never larger than about one part in 1010) in the EFT's regime of validity, this work has interesting theoretical implications for our understanding of general relativity and lays the groundwork for future studies on superradiant phenomena in binary systems.