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From the 2 of 22 linked papers with an AI index.

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20242026
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22 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

Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks

Jiaxi Wu, Elias R. Most, Nils L. Vu +4

In this work, we investigate gravitational-wave signatures of a proposed subsolar-mass merger scenario resulting from fragmentation inside a collapsar accretion disk. This scenario…

gr-qc2026

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries

Adhrit Ravichandran, Peter James Nee, Keefe Mitman +22

Accurate models of merger remnants are increasingly important for gravitational-wave science, including precision tests of gravity with ringdown, inference of black-hole population…

gr-qc2026

Learning Post-Newtonian Corrections from Numerical Relativity

Jooheon Yoo, Michael Boyle, Nils Deppe

Accurate modeling of gravitational waveforms from compact binary coalescences remains central to gravitational-wave (GW) astronomy. Post-Newtonian (PN) approximations capture the e…

gr-qc2025

Error quantification and comparison of binary neutron star gravitational waveforms from numerical relativity codes

Sarah Habib, Elias R. Most, Nils Deppe +11

Future gravitational wave detections of merging binary neutron star systems have the possibility to tightly constrain the equation of state of dense nuclear matter. In order to ext…