Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

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2010

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2018

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2018

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2018

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2018

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2018

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2019

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2021

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Tousif Islam, Vijay Varma, Jackie Lodman, Scott E. Field, Gaurav Khanna, Mark A. Scheel, Harald P. Pfeiffer, Davide Gerosa, and Lawrence E. Kidder, “Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case,” Phys. Rev. D 103

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2021

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2021

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2021

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Vijay Varma, Sylvia Biscoveanu, Tousif Islam, Feroz H Shaik, Carl-Johan Haster, Maximiliano Isi, Will M Farr, Scott E Field, and Salvatore Vitale, “Evidence of large recoil velocity from a black hole merger signal,” Physical Review Letters 128

2022

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Alessandro Nagar, James Healy, Carlos O. Lousto, Sebastiano Bernuzzi, and Angelica Albertini, “Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime,” (2022), arXiv:2202.05643 [gr-qc]

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2022

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Jooheon Yoo, Vijay Varma, Matthew Giesler, Mark A. Scheel, Carl-Johan Haster, Harald P. Pfeiffer, Lawrence E. Kidder, and Michael Boyle, “Targeted large mass ratio numerical relativity surrogate waveform model for GW190814,” Phys. Rev. D 106

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2022

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Carlos O. Lousto and James Healy, “Study of the Intermediate Mass Ratio Black Hole Binary Merger up to 1000:1 with Numerical Relativity,” (2022), arXiv:2203.08831 [gr-qc]

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2022

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Matthew Giesler, Mark A. Scheel, and Saul A. Teukolsky, “Numerical simulations of extreme mass ratio binary black holes,” (2022), in preparation

2022

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Tousif Islam, Scott E. Field, Scott A. Hughes, Gaurav Khanna, Vijay Varma, Matthew Giesler, Mark A. Scheel, Lawrence E. Kidder, and Harald P. Pfeiffer, “Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity,” Phys. Rev. D 106

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2022

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