Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries
By P. Ajith, Stanislav Babak, Yi Chen, M. Hewitson, B. Krishnan, A. Sintes, J. Whelan, B. Brügmann, Peter Diener, N. Dorband and 8 more. 2008
247 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/a451eb9a943c4072e38a6159fadec384e444f519
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In Astronomy and Astrophysics
- Luciano Rezzolla
- E. Barausse
- B. Kelly
- J. V. Meter
- J. Centrella
- John G. Baker
- Fabian Hofmann
- Ilya Mandel
Citations in the corpus
- Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, unknown): “[7, 74, 82, 91, 92] for more details.”
- Gravitational waves from neutron star mergers and their relation to the nuclear equation of state (2019, methodology): “ee the end of Sect. 4.2 and Sect. 5 for related work). A few types of waveform models have become the standard in GW analysis: post-Newtonian, eective-one-body (EOB) [449, 450] and the Phenom models [451, 452]. Post-Newtonian expansions are approximate solutions, valid for weaker elds, of the Einste”
- THE FINAL SPIN FROM BINARY BLACK HOLES IN QUASI-CIRCULAR ORBITS (2016, methodology): “…Frankfurt, Germany tion are employed, e.g., the spin-effective-one-body (sEOB) model (Buonanno & Damour 1999; Damour 2001; Barausse & Buonanno 2010) or “hybrid” waveforms (Ajith et al. 2008; Khan et al. 2015), which combine results from NR simulations with PN and quasinormal-mode calculations.”
- Surrogate model of hybridized numerical relativity binary black hole waveforms (2018, background): “Different blending functions have been proposed in the literature [60, 63, 65, 91].”
- Compact binary coalescences in the band of ground-based gravitational-wave detectors (2009, background): “Similarly, astrophysical input can aid decisions regarding the allocation of limited human and computational resources in data analysis: Should searches be expanded to the mass range of intermediate-mass black holes? Given scarce resources, does it make sense to develop a new search for eccentric bi”