[PDF] Top 20 BPASS predictions for binary black hole mergers

... multiple high probability regions rather than a single field (Singer et al. 2014; Essick et al. 2015). Identification of counterparts in such large regions is exceptionally difficult due both to the small field of view ... See full document

... model predictions, in particular merger rates, but also probability distributions of BBH properties, are affected by a considerable number of physical factors and associated parameters, albeit at different levels ... See full document

... of black holes and compact objects like neutron stars and theoretical advancements gave impetus to the ...the mergers of binary compact objects, like binary neutron stars as well as ... See full document

... inner binary of a stable hierarchical triple system ) , the KL mechanism triggers oscillations of the BBH ’ s eccentricity, which might speed up the merger by gravitational-wave ...produce black hole ... See full document

... To observe CBCs in data taken from Advanced LIGO we use matched- fi ltering against models of compact binary merger gravitational-wave ( GW ) signals ( Wainstein & Zubakov 1962 ) . Matched- fi ltering has long ... See full document

... and black holes and it forms the basis of our understanding of ...its predictions is the existence of gravitational waves (GW), which are a strain of spacetime propogating at the speed of ...the ... See full document

... Two independent pipelines searched the coincident data for signals matching a compact binary coalescence ( CBC; Abbott et al. 2016c ) , each producing a set of coincident search triggers. Both the pycbc pipeline ( ... See full document

... This article provides supplemental information for a Letter reporting the rate of ( BBH ) coalescences inferred from 16 days of coincident Advanced LIGO observations surrounding the transient ( GW ) signal GW150914. In ... See full document

... , (13) where A is an amplitude factor that depends on the intrinsic properties (source-frame masses and spins) of the source, the detector sensitivity expressed as a noise power spectral density S(f) as a function of ... See full document

... a black hole [5,6], and in 1963 Kerr generalized the solution to rotating black holes ...of black hole quasinormal modes [8 – 10], and in the 1990s higher-order post- Newtonian ... See full document

... a black hole [5,6], and in 1963 Kerr generalized the solution to rotating black holes ...of black hole quasinormal modes [8 – 10], and in the 1990s higher-order post- Newtonian ... See full document

... two black holes has proven to be remarkably ...colliding black holes [32] to compute the gravitational- wave signal from the last orbits, merger, and ringdown of a black-hole binary ... See full document

... As was mentioned previously, a reliable upper limit cannot be calculated for the rate of BBH inspirals as was calculated for the rate of BNS inspirals. The reason for this is twofold. First, the characteristics of the ... See full document

... (NS) mergers following the confirmation by hydrodynamic simulations that a non-negligible amount of matter can be ejected and by nucleosynthesis calculations combined with the predicted astrophysical event rate ... See full document

... super-massive black hole (SMBH) binary in the limit of a thin ...given black hole spins aligned or anti-aligned with the orbital angular momentum, mass-energy loss is the dominant effect ... See full document

... for binary black hole (BBH) systems in theories beyond ...BBH mergers in dynamical Chern-Simons gravity (dCS) to linear order in the perturbation ...analytic predictions at early times, ... See full document

... stellar-mass binary black holes ...compact binary coalescence (CBC) search targets gravita- tional-wave emission from compact-object binaries with individual masses from 1 M ⊙ to 99 M ⊙ , total mass ... See full document

... the binary; this is meant to be a quasiequilibrium condition that reduces initial gauge ...for mergers, so SpEC simulations customarily move from co-rotating gauge to damped harmonic gauge via a smooth ... See full document

... or black holes are expected to be the main signals detected by the advanced generation of gravitational wave detectors [35, 36, 157, ...compact binary waveforms. A compact binary intrinsically ... See full document

... generality by large-scale NR simulations [32 – 34]. Since these pioneering works, numerous improvements have enabled numerical simulations of BBHs with sufficient accuracy for the applications considered here and for the ... See full document