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The current paradigm for constructing waveforms from precessing compact binaries is to first construct a waveform in a non-inertial, co-precessing binary source frame followed by a time-dependent rotation to map back to the physical, inertial frame.
1903
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2008
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2008
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Bernd Brügmann, José A. González, Mark Hannam, Sascha Husa, Ulrich Sperhake, and Wolfgang Tichy, “Calibration of moving puncture simulations,” Phys. Rev. D 77
2008
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2014
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2008
Cited alongside, same era.
K. G. Arun, Alessandra Buonanno, Guillaume Faye, and Evan Ochsner, “Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms,” Phys. Rev. D 79
2009
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Michael Boyle and Abdul H. Mroué, “Extrapolating gravitational-wave data from numerical simulations,” Phys. Rev. D 80
2009
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2009
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M Punturo et al. , “The einstein telescope: a third-generation gravitational wave observatory,” Classical and Quantum Gravity 27
2010
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2010
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Patricia Schmidt, Mark Hannam, Sascha Husa, and P. Ajith, “Tracking the precession of compact binaries from their gravitational-wave signal,” Phys. Rev. D 84
2011
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R. O’Shaughnessy, B. Vaishnav, J. Healy, Z. Meeks, and D. Shoemaker, “Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation,” Phys. Rev. D 84
2011
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S. Khan, S. Husa, M. Hannam, F. Ohme, M. Pürrer, F. Jiménez Forteza, and A. Bohé, “Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era,” (2015)
2015
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Patricia Schmidt, Frank Ohme, and Mark Hannam, “Towards models of gravitational waveforms from generic binaries: Ii. modelling precession effects with a single effective precession parameter,” Phys. Rev. D 91
2015
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Jonathan Blackman, Scott E. Field, Chad R. Galley, Bela Szilagyi, Mark A. Scheel, et al. , “Fast and accurate prediction of numerical relativity waveforms from binary black hole mergers using surrogate models,” (2015)
2015
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John Miller, Lisa Barsotti, Salvatore Vitale, Peter Fritschel, Matthew Evans, and Daniel Sigg, “Prospects for doubling the range of advanced ligo,” Phys. Rev. D 91
2015
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B. P. et al Abbott (LIGO Scientific Collaboration and Virgo Collaboration), “Observation of gravitational waves from a binary black hole merger,” Phys. Rev. Lett. 116
2016
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Sascha Husa, Sebastian Khan, Mark Hannam, Michael Pürrer, Frank Ohme, Xisco Jiménez Forteza, and Alejandro Bohé, “Frequency-domain gravitational waves from nonprecessing black-hole binaries. i. new numerical waveforms and anatomy of the signal,” Phys. Rev. D 93
2016
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A. Bohé et al. , PhenomPv2 - Technical Notes for LAL Implementation , Tech. Rep. LIGO-T1500602 (2016)
2016
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2017
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Xisco Jiménez-Forteza, David Keitel, Sascha Husa, Mark Hannam, Sebastian Khan, and Michael Pürrer, “Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy,” Phys. Rev. D 95
2017
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B P Abbott et al. , “Exploring the sensitivity of next generation gravitational wave detectors,” Classical and Quantum Gravity 34
2017
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Stanislav Babak, Andrea Taracchini, and Alessandra Buonanno, “Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity,” Phys. Rev. D 95
2017
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2018
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Lionel London, Sebastian Khan, Edward Fauchon-Jones, Cecilio García, Mark Hannam, Sascha Husa, Xisco Jiménez-Forteza, Chinmay Kalaghatgi, Frank Ohme, and Francesco Pannarale, “First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries,” Phys. Rev. Lett. 120
2018
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Roberto Cotesta, Alessandra Buonanno, Alejandro Bohé, Andrea Taracchini, Ian Hinder, and Serguei Ossokine, “Enriching the symphony of gravitational waves from binary black holes by tuning higher harmonics,” Phys. Rev. D 98
2018
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2019
Later among the works it cites.
Maria Babiuc-Hamilton et al. , “The Einstein Toolkit,” (2019), to find out more, visit http://einsteintoolkit.org
2019
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Antoni Ramos-Buades, Sascha Husa, and Geraint Pratten, “Simple procedures to reduce eccentricity of binary black hole simulations,” Phys. Rev. D 99
2019
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Geraint Pratten et al, (2020), in preparation
2020
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Héctor Estellés, Antoni Ramos-Buades, Sascha Husa, Cecilio García-Quirós, and Leila Haegel, “IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes,” (2020), in preparation
2020
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Jeffrey Bowen and James York, “Time-asymmetric initial data for black holes and black-hole collisions,” Phys. Rev. D 21
2056
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Jeffrey M. Bowen and James W. York, “Time-asymmetric initial data for black holes and black-hole collisions,” Phys. Rev. D 21
2056
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