Critical behavior in Ricci flow

David Garfinkle; James Isenberg

Critical behavior in Ricci flow

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 math/0306129 v1 pith:FIWXHHQK submitted 2003-06-07 math.DG gr-qc

Critical behavior in Ricci flow

David Garfinkle , James Isenberg This is my paper

classification math.DG gr-qc

keywords riccibehaviorcriticalflowformationamountscomparingcorresponding

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

We use numerical techniques to study the formation of singularities in Ricci flow. Comparing the Ricci flows corresponding to a one parameter family of initial geometries on S^3 with varying amounts of S^2 neck pinching, we find critical behavior at the threshold of singularity formation.

discussion (0)

Forward citations

Cited by 1 Pith paper

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

Dynamical Boson Stars
gr-qc 2012-02 unverdicted novelty 2.0

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.