Pith. sign in

REVIEW 1 cited by

The Wave Equation on Extreme Reissner-Nordstr\"om Black Hole Spacetimes: Stability and Instability Results

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 1006.0283 v2 pith:OZN3B42H submitted 2010-06-02 math.AP gr-qcmath-phmath.DGmath.MP

classification math.APgr-qcmath-phmath.DGmath.MP
keywords eventhorizonequationextremeresultswaveanalyticalarising
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We consider solutions to the linear wave equation on a suitable globally hyperbolic subset of an extreme Reissner-Nordstrom spacetime, arising from regular initial data prescribed on a Cauchy hypersurface crossing the future event horizon. We obtain boundedness, decay, non-decay and blow-up results. Our estimates hold up to and including the event horizon. The fundamental new aspect of this problem is the degeneracy of the redshift on the event horizon. Several new analytical features of degenerate horizons are also presented.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Newman-Penrose-like exact and approximate conservation laws: a covariant and conformal formulation

    gr-qc 2025-07 conditional novelty 7.0 of 10

    A conformal spin-coefficient formalism gives a covariant derivation of Newman-Penrose conservation laws for massless fields, proves Aretakis charges on extremal horizons, and yields approximate conservation laws in sp...

Pith tools