Dynamical descalarization with a jump during a black hole merger
نویسندگان
چکیده
Black holes in scalar-Gauss-Bonnet gravity are prone to scalarization, that is a spontaneous development of scalar hair for strong enough spacetime curvature while the weak field regime theory coincides with general relativity. Since large associated smaller black hole masses, merging can lead dynamical descalarization. This release newly formed case its mass above scalarization threshold. Depending on exact form Gauss-Bonnet coupling function, stable scalarized solutions be either continuously connected Schwarzschild hole, or transitions between two happen jump. By performing simulations head-on collisions descalization, we have demonstrated such jump clearly observed accumulated gravitational wave data multiple merger events different masses. The distinct signature signal will share similarities effects expected from first order matter phase happening during neutron star binary mergers.
منابع مشابه
Supermassive Black Hole Merger Rates: Uncertainties from Halo Merger Theory
The merger of two supermassive black holes is expected to produce a gravitational-wave signal detectable by the satellite LISA. The rate of supermassive-black-hole mergers is intimately connected to the halo merger rate, and the extended Press–Schechter formalism is often employed when calculating the rate at which these events will be observed by LISA. This merger theory is flawed and provides...
متن کاملObservation of Gravitational Waves from a Binary Black Hole Merger
This cataclysmic event, producing the gravitational-wave signal GW150914, took place in a distant galaxy more than one billion light years from the Earth. It was observed on September 14, 2015 by the two detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO), arguably the most sensitive scientific instruments ever constructed. LIGO estimated that the peak gravitational-wave...
متن کاملBinary black hole merger dynamics and waveforms
We study dynamics and radiation generation in the last few orbits and merger of a binary black hole system, applying recently developed techniques for simulations of moving black holes. Our analysis of the gravitational radiation waveforms and dynamical black hole trajectories produces a consistent picture for a set of simulations with black holes beginning on circular-orbit trajectories at a v...
متن کاملComparisons of binary black hole merger waveforms
John G. Baker, Manuela Campanelli, 3 Frans Pretorius, 5, 6 and Yosef Zlochower Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA Center for Gravitational Wave Astronomy, Department of Physics and Astronomy, The University of Texas at Brownsville, Brownsville, Texas 78520 Center for Computational Relativity and Gravitation, Scho...
متن کاملObservation of Gravitational Waves from a Binary Black Hole Merger
This cataclysmic event, producing the gravitational-wave signal GW150914, took place in a distant galaxy more than one billion light years from the Earth. It was observed on September 14, 2015 by the two detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO), arguably the most sensitive scientific instruments ever constructed. LIGO estimated that the peak gravitational-wave...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physical review
سال: 2022
ISSN: ['0556-2813', '1538-4497', '1089-490X']
DOI: https://doi.org/10.1103/physrevd.106.l061502