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From the 2 of 32 linked papers with an AI index.

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20242026
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32 papers

gr-qc2026

High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach

Guillermo Lara, Harald P. Pfeiffer, Nils Deppe +9

The paper implements a fixing‑the‑equations method in the Spectre code to generate accurate numerical‑relativity waveforms for black‑hole binaries in shift‑symmetric scalar Gauss‑B…

gr-qc2026

Towards long and accurate numerical relativity waveforms of binary black holes beyond general relativity

Guillermo Lara, Harald P. Pfeiffer, Nils Deppe +9

The paper presents long, accurate numerical relativity simulations of equal‑mass, nonspinning binary black holes in shift‑symmetric scalar Gauss‑Bonnet gravity, generating waveform…

astro-ph.HE2026

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers

Francois Foucart, Samantha Rath, Rowan Davidson +5

Multimessenger observations of neutron star mergers are unique opportunities to constrain the properties of dense matter and the production site of heavy nuclei. To leverage these…

gr-qc2026

A comprehensive look into the accuracy of SpEC binary black hole waveforms

Taylor Knapp, Katerina Chatziioannou, Keefe Mitman +4

Numerical relativity simulations provide a full description of the dynamics of binary systems, including gravitational radiation. The waveforms produced by these simulations have a…

astro-ph.HE2026

Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars

Samantha Rath, Francois Foucart, Lawrence E. Kidder +2

Neutron star mergers are amongst the most promising sources for the joint detection of gravitational waves and electromagnetic signals. They are also potential sites for the produc…

gr-qc2026

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM

Aldo Gamboa, Alessandra Buonanno, Lorenzo Pompili +8

Accurate and computationally efficient waveform models are required to infer the parameters of compact binaries from their gravitational wave (GW) emission. Among these parameters,…