Soliton resolution for equivariant wave maps on a wormhole: II
Casey Rodriguez

TL;DR
This paper proves the soliton resolution conjecture for equivariant wave maps on a wormhole spacetime, showing that solutions decompose into a harmonic map plus radiation, thus advancing understanding of wave map dynamics in complex geometries.
Contribution
It establishes the soliton resolution for equivariant wave maps on a wormhole, extending previous results to a broader class of equivariance and confirming a conjecture by Bizon and Kahl.
Findings
Solutions decompose into harmonic map plus radiation
Convergence to stable harmonic maps is proven
Fully resolves the soliton resolution conjecture for this model
Abstract
In this paper, we continue our study of equivariant \emph{wave maps on a wormhole} initiated in our companion paper. More precisely, we study finite energy --equivariant wave maps from the (1+3)-dimensional spacetime where the metric on is given by \begin{align*} ds^2 = -dt^2 + dr^2 + (r^2 + 1) \left ( d \theta^2 + \sin^2 \theta d \varphi^2 \right ), \quad t,r \in \mathbb R, (\theta,\varphi) \in \mathbb{S}^2. \end{align*} The constant time slices are each given by a Riemannian manifold with two asymptotically Euclidean ends at that are connected by a 2--sphere at . The spacetime has appeared in the general relativity literature as a prototype wormhole geometry (but is…
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Taxonomy
TopicsAdvanced Mathematical Physics Problems · Black Holes and Theoretical Physics · Nonlinear Waves and Solitons
