Pith. sign in

REVIEW 3 cited by

The RIT binary black hole simulations catalog

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1703.03423 v1 pith:KFXMQ6QH submitted 2017-03-09 gr-qc astro-ph.COastro-ph.HE

The RIT binary black hole simulations catalog

James Healy , Carlos O. Lousto , Yosef Zlochower , Manuela Campanelli (CCRG-RIT) This is my paper
classification gr-qc astro-ph.COastro-ph.HE
keywords catalogwaveformsblackholeinformationinitialprecessingsimulations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The RIT numerical relativity group is releasing a public catalog of black-hole-binary waveforms. The initial release of the catalog consists of 126 recent simulations that include precessing and non precessing systems with mass ratios $q=m_1/m_2$ in the range $1/6\leq q\leq1$. The catalog contains information about the initial data of the simulation, the waveforms extrapolated to infinity, as well as information about the peak luminosity and final remnant black hole properties. These waveforms can be used to independently interpret gravitational wave signals from laser interferometric detectors and

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Spontaneous spherical symmetry breaking of black holes with resonant hair

    gr-qc 2026-04 accept novelty 6.0

    Black holes with resonant scalar hair are dynamically unstable in 3+1 numerical relativity, decaying via fission or absorption into bald black holes.

  2. Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity

    gr-qc 2024-07 conditional novelty 6.0

    BHPTNRSur2dq1e3 is a new surrogate model for spinning intermediate-mass-ratio black hole binary gravitational waves, constructed from ppBHPT training data with domain decomposition for retrograde modes and calibrated ...

  3. Spontaneous spherical symmetry breaking of black holes with resonant hair

    gr-qc 2026-04 unverdicted novelty 5.0

    Black holes with resonant hair spontaneously break spherical symmetry and decay into bald black holes via non-spherical dynamics, either through fission or absorption.