Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
Jooheon Yoo, Keefe Mitman, Vijay Varma, Michael Boyle, Scott E. Field,, Nils Deppe, Fran\c{c}ois H\'ebert, Lawrence E. Kidder, Jordan Moxon, Harald, P. Pfeiffer, Mark A. Scheel, Leo C. Stein, Saul A. Teukolsky, William Throwe,, and Nils L. Vu

TL;DR
This paper introduces a new gravitational waveform surrogate model built from Cauchy-characteristic evolution waveforms, accurately capturing memory effects and hybridized with post-Newtonian and effective one-body waveforms for binary black hole mergers.
Contribution
The paper presents NRHybSur3dq8_CCE, a novel surrogate model that incorporates memory effects by using CCE waveforms and hybridization, improving physical accuracy over previous models.
Findings
Achieves mismatches less than 2e-4 for a wide mass range
Successfully captures gravitational memory effects
Models waveforms for mass ratios up to 8 and spins within [-0.8, 0.8]
Abstract
Numerical relativity simulations provide the most precise templates for the gravitational waves produced by binary black hole mergers. However, many of these simulations use an incomplete waveform extraction technique -- extrapolation -- that fails to capture important physics, such as gravitational memory effects. Cauchy-characteristic evolution (CCE), by contrast, is a much more physically accurate extraction procedure that fully evolves Einstein's equations to future null infinity and accurately captures the expected physics. In this work, we present a new surrogate model, NRHybSur3dq8CCE, built from CCE waveforms that have been mapped to the post-Newtonian (PN) BMS frame and then hybridized with PN and effective one-body (EOB) waveforms. This model is trained on 102 waveforms with mass ratios and aligned spins . The…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Model Reduction and Neural Networks
