DOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES

By M. Dominik, Emanuele Berti, R. O’Shaughnessy, Ilya Mandel, Krzysztof Belczyński, Chris L. Fryer, D. Holz, T. Bulik, F. Pannarale. 2015

273 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/b5f054047ef3857676ea67d1098eb1d09ce27b80

Citations in the corpus

• Where Are LIGO’s Big Black Holes? (2017, unknown): “We then generate random angular factors, 0 < w < 1, from a single-detector antenna power pattern, assuming that binaries are distributed uniformly on the sky with isotropic inclination vectors (Finn & Chernoff 1993; Dominik et al. 2015; Belczynski et al. 2016b).”
• Double neutron stars: merger rates revisited (2017, unknown): “…M ), but is relevant for massive stars, as revealed by observational studies ( fbin = 1, e.g. Sana et al. 2012) Note that this is different than in Dominik et al. (2012, 2013, 2015); Chruslinska et al. (2017) where fbin = 0.5 was used in the whole mass range and leads to nearly twice higher…”
• The cosmic merger rate of neutron stars and black holes (2018, unknown): “As to DNS mergers, population-synthesis simulations have been used to predict merging rates spanning from few tens to several hundreds mergers Gpc−3 yr−1 (e.g. Abadie et al. 2010; Dominik et al. 2013, 2015; Ziosi et al. 2014; de Mink & Belczynski 2015).”
• Assisted inspirals of stellar mass black holes embedded in AGN discs: solving the ‘final au problem’ (2016, unknown): “For instance, Dominik et al. (2015) predict a rate of ∼ 1 − 100 Gpc−3 yr−1, with a median chirp mass of 15−25M .”
• Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries (2015, unknown): “The mass distribution shows greater support for high masses than either classical population-synthesis predictions for field binary black holes (e.g. Dominik et al. 2015) or dynamically formed binary black hole models in globular clusters (e.g. Rodriguez et al. 2015).”
• Measuring the Binary Black Hole Mass Spectrum with an Astrophysically Motivated Parameterization (2018, unknown): “These works range from comparing gravitationalwave data to specific, non-parameterized models (Mandel & O’Shaughnessy 2010; Dominik et al. 2015; Stevenson et al. 2015, 2017a; Belczynski et al. 2016, 2017; Barrett et al. 2017; Farr et al. 2017; Miyamoto et al. 2017; Wysocki et al. 2018; Zevin et al.…”
• Black Hole Mergers From Globular Clusters Observable by LISA I: Eccentric Sources Originating From Relativistic N-body Dynamics (2018, unknown): “From a theoretical perspective, several formation channels have been suggested including isolated field binaries (Dominik et al. 2012, 2013, 2015; Belczynski et al. 2016b,a), dense stellar clusters (Portegies Zwart & McMillan 2000; Banerjee et al. 2010; Tanikawa 2013; Bae et al. 2014; Rodriguez et…”
• A new route towards merging massive black holes (2016, unknown): “…binaries are produced through common-envelope evolution (see Appendix B), except for a few cases (Voss & Tauris 2003; Belczynski et al. 2010; Dominik et al. 2015), the far majority of published population synthesis studies predict a much higher NS+NS merger rate per Milky Way equivalent…”
• COMPACT BINARY MERGER RATES: COMPARISON WITH LIGO/VIRGO UPPER LIMITS (2015, unknown): “Following Dominik et al. (2013; 2015) we consider four evolutionary models (see Table 1 for model summaries).”
• Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA (2013, unknown): “…rate estimation based upon astrophysical population models and observations of Galactic BNS systems (e.g., Abadie et al. 2010b; Kim et al. 2013; Dominik et al. 2015; Vangioni et al. 2016; de Mink and Belczynski 2015; Eldridge et al. 2017; Belczynski et al. 2017; Kruckow et al. 2018) remains an…”
• The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks (2018, unknown): “…Tauris & van den Heuvel 2006; Portegies Zwart & Yungelson 1998; Portegies Zwart & McMillan 2000; Belczynski et al. 2007; Bogomazov et al. 2007; Dominik et al. 2012, 2013, 2015; Mennekens & Vanbeveren 2014; Tauris et al. 2015, 2017; de Mink & Belczynski 2015; de Mink & Mandel 2016; Marchant et…”
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo (2013, unknown): “, [69, 50, 49, 47]), and will be informed by the number of detections (or lack thereof) in observing runs.”
• Progenitors of gravitational wave mergers: binary evolution with the stellar grid-based code ComBinE (2018, unknown): “There are several binary population synthesis studies performed with the codes StarTrack (Belczynski et al. 2008; Dominik et al. 2013, 2015; Chruslinska et al. 2018), binary c (Izzard et al. 2004, 2006, 2009, 2018), BPASS (Eldridge & Stanway 2016; Eldridge et al. 2017), COMPAS (Stevenson et al.…”