REVIEW 2 cited by
Dispersive estimates for Dirac equations in Aharonov-Bohm magnetic fields: massless case
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
read the original abstract
In this paper we study the dispersive properties of a two dimensional massless Dirac equation perturbed by an Aharonov--Bohm magnetic field. Our main results will be a family of pointwise decay estimates and a full range family Strichartz estimates for the flow. The proof relies on the use of a relativistic Hankel transform, which allows for an explicit representation of the propagator in terms of the generalized eigenfunctions of the operator. These results represent the natural continuation of earlier research on evolution equations associated to operators with magnetic fields with strong singularities (see \cite{DF, FFFP, FZZ} where the Schr\"odinger and the wave equations were studied). Indeed, we recall the fact that the Aharonov--Bohm field represents a perturbation which is critical with respect to the scaling: this fact, as it is well known, makes the analysis particularly challenging.
Forward citations
Cited by 2 Pith papers
-
Decay and Strichartz estimates for critical electromagnetic wave equations on conic manifolds
The authors establish microlocalized pointwise decay and Strichartz estimates for electromagnetic wave equations on n-dimensional product cones, with the admissible p-range restricted by the smallest eigenvalue of the...
-
Pointwise dispersive estimates for Schrodinger and wave equations in a conical singular space
On product cones over closed manifolds with conjugate radius larger than pi, the Schrödinger and half-wave propagators satisfy global pointwise dispersive estimates with the Euclidean decay rate times an angular weight.
Discussion (0). Continue with ORCID to comment.