Pith. sign in

REVIEW 3 cited by

Late-Time Behavior of Stellar Collapse and Explosions: II. Nonlinear Evolution

Not yet reviewed by Pith; the record is open.

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 gr-qc/9307010 v2 pith:FAY3BMYI submitted 1993-07-10 gr-qc astro-ph

Late-Time Behavior of Stellar Collapse and Explosions: II. Nonlinear Evolution

classification gr-qc astro-ph
keywords apparentlybehaviorbrokencausecollapsecorrectedevolutionexplosions
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Problem with the figures should be corrected. Apparently a broken uuencoder was the cause.

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. Parametrized beyond-Teukolsky framework in the time domain

    gr-qc 2026-07 conditional novelty 6.0

    First time-domain implementation of the parametrized beyond-Teukolsky framework, validated against frequency-domain benchmarks for low multipoles and yielding new amplitude, phase, quadratic-coefficient, and tail-onse...

  2. On the universality of late-time ringdown tail

    gr-qc 2025-05 unverdicted novelty 6.0

    Analytical proof establishes universality of late-time ringdown tails for any effective potential decaying as 1/r², with different power-law behavior for 1/r^α (1<α<2), covering charged black holes, Kerr, exotic objec...

  3. Quasi-Normal Modes of Stars and Black Holes

    gr-qc 1999-09 unverdicted novelty 2.0

    A review summarizing the properties, calculation methods, and astrophysical relevance of quasi-normal modes for Schwarzschild, Reissner-Nordström, Kerr, Kerr-Newman black holes and non-rotating or slowly-rotating stars.