Pith. sign in

REVIEW 2 cited by

Evidence for violations of Weak Cosmic Censorship in black hole collisions in higher dimensions

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 2011.03049 v2 pith:F5544NNW submitted 2020-11-05 hep-th gr-qc

classification hep-thgr-qc
keywords blackevidenceholescensorshipcollisionscosmicdimensionshigher
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
abstract

We study collisions of boosted rotating black holes in $D=6$ and 7 spacetime dimensions with a non-zero impact parameter. We find that there exists an open set of initial conditions such that the intermediate state of the collision is a black hole with a dumbbell-like horizon which is unstable to a local Gregory-Laflamme-type instability. We are able to provide convincing numerical evidence that the evolution of such an instability leads to a pinch off of the horizon in finite asymptotic time thus forming a naked singularity, as in similar unstable black holes. Since the black holes in the initial state are stable, this is the first genuinely generic evidence for the violation of the Weak Cosmic Censorship Conjecture in higher dimensional asymptotically flat spacetimes.

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. Cosmic censorship in a (dual) collider

    hep-th 2024-11 conditional novelty 6.0 of 10

    In holographic models with a good-singularity ground state, a boost-invariant expanding fluid drives the dual horizon curvature to diverge in classical gravity.

  2. A smooth road to bumpy horizons: shaping black holes with non-linear sigma models, from supergravity to higher dimensions

    hep-th 2026-03 conditional novelty 5.0 of 10

    Potential-free non-linear sigma models in General Relativity support static 'bumpy-horizon' black holes, with the horizon conformal factor determined by an inhomogeneous Liouville equation sourced by arbitrary holomor...

Pith tools