Pith. sign in

REVIEW 2 cited by

An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries

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 2110.09254 v3 pith:DTEJF5T6 submitted 2021-09-28 astro-ph.HE gr-qc

Ilya Mandel This is my paper · ORCID
classification astro-ph.HEgr-qc
keywords accurateanalyticaldurationgravitational-waveinspiralbinariesdriveneccentric
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

I present an analytical fit to the duration of the inspiral of two point masses driven by gravitational-wave emission. The fit is accurate to within 3% over the entire range of initial eccentricities from 0 to 0.99999.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Stable mass transfer in massive binaries leading to merging black holes

    astro-ph.SR 2025-12 conditional novelty 7.0 of 10

    Stable mass transfer in massive binaries, modeled with the accreting star's altered structure, produces merging black holes matching LIGO/Virgo masses and spins.

  2. Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    Single intermediate-mass black hole mergers detected by next-generation observatories cannot pin down progenitor cluster mass or radius because of model degeneracy, but formation redshift posteriors are narrow enough ...

Pith tools