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We study co--rotational wave maps from $(3+1)$--Minkowski space to the three--sphere $S^3$. It is known that there exists a countable family $\{f_n\}$ of self--similar solutions. We investigate their stability under linear perturbations by…

Mathematical Physics · Physics 2009-08-01 Roland Donninger , Peter C. Aichelburg

We study numerically the Cauchy problem for equivariant wave maps from 3+1 Minkowski spacetime into the 3-sphere. On the basis of numerical evidence combined with stability analysis of self-similar solutions we formulate two conjectures.…

Mathematical Physics · Physics 2009-10-31 P. Bizoń , T. Chmaj , Z. Tabor

We consider the exterior Cauchy-Dirichlet problem for equivariant wave maps from 3+1 dimensional Minkowski spacetime into the three-sphere. Using mixed analytical and numerical methods we show that, for a given topological degree of the…

Mathematical Physics · Physics 2015-05-30 Piotr Bizoń , Tadeusz Chmaj , Maciej Maliborski

We study linear perturbations of a self-similar wave map from Minkowski space to the three-sphere which is conjectured to be linearly stable. Considering analytic mode solutions of the evolution equation for the perturbations we prove that…

Mathematical Physics · Physics 2008-11-26 Roland Donninger , Peter C. Aichelburg

We study corotational wave maps from $(1+3)$-dimensional Minkowski space into the three-sphere. We establish the asymptotic stability of an explicitly known self-similar wave map under perturbations that are small in the critical Sobolev…

Analysis of PDEs · Mathematics 2025-04-02 Roland Donninger , David Wallauch

We consider co-rotational wave maps from (3+1) Minkowski space into the three-sphere. This is an energy supercritical model which is known to exhibit finite time blow up via self-similar solutions. The ground state self-similar solution…

Analysis of PDEs · Mathematics 2012-01-31 Roland Donninger , Birgit Schoerkhuber , Peter C. Aichelburg

In this thesis the Cauchy problem and in particular the question of singularity formation for co--rotational wave maps from 3+1 Minkowski space to the three--sphere $S^3$ is studied. Numerics indicate that self--similar solutions of this…

Mathematical Physics · Physics 2007-11-28 Roland Donninger

In this paper we report on numerical studies of the Cauchy problem for equivariant wave maps from 2+1 dimensional Minkowski spacetime into the two-sphere. Our results provide strong evidence for the conjecture that large energy initial data…

Mathematical Physics · Physics 2009-10-31 Piotr Bizoń , Tadeusz Chmaj , Zbislaw Tabor

We consider wave maps from $(1+d)$-dimensional Minkowski space, $d\geq3$, into rotationally symmetric manifolds which arise from small perturbations of the sphere $\mathbb S^d$. We prove the existence of co-rotational self-similar finite…

Analysis of PDEs · Mathematics 2025-03-07 Roland Donninger , Birgit Schörkhuber , Alexander Wittenstein

We consider wave maps from $(1+d)$-dimensional Minkowski space into the $d$-sphere. For every $d \geq 3$, there exists an explicit self-similar solution that exhibits finite time blowup. This solution is corotational and its mode stability…

Analysis of PDEs · Mathematics 2026-04-16 Roland Donninger , Frederick Moscatelli

In this paper we study 1-equivariant wave maps of finite energy from 1+3-dimensional Minkowski space exterior to the unit ball at the origin into the 3-sphere. We impose a Dirichlet boundary condition at r=1, meaning that the unit sphere in…

Analysis of PDEs · Mathematics 2013-12-19 Carlos Kenig , Andrew Lawrie , Wilhelm Schlag

We consider co--rotational wave maps from (3+1) Minkowski space into the three--sphere. This is an energy supercritical model which is known to exhibit finite time blow up via self-similar solutions. The ground state self--similar solution…

Analysis of PDEs · Mathematics 2011-05-25 Roland Donninger

Consider the equivariant wave map equation from Minkowski space to a rotationnally symmetric manifold which has an equator (example: the sphere). In dimension 3, this article gives a necessary and sufficient condition for the existence of a…

Analysis of PDEs · Mathematics 2008-06-26 Pierre Germain

We prove that the focusing cubic wave equation in three spatial dimensions has a countable family of self-similar solutions which are smooth inside the past light cone of the singularity. These solutions are labeled by an integer index $n$…

Analysis of PDEs · Mathematics 2011-04-07 P. Bizoń , P. Breitenlohner , D. Maison , A. Wasserman

The author gives an alternative and simple proof of the global existence of smooth solutions to the Cauchy problem for wave maps from the 1+2-dimensional Minkowski space to an arbitrary compact smooth Riemannian manifold without boundary,…

Analysis of PDEs · Mathematics 2023-02-21 Yi Zhou

In this paper we consider the equation for equivariant wave maps from $R^{3+1}$ to $S^3$ and we prove global in forward time existence of certain $C^\infty$-smooth solutions which have infinite critical Sobolev norm…

Analysis of PDEs · Mathematics 2016-08-01 Elisabetta Chiodaroli , Joachim Krieger

We show that wave maps $\phi$ from two-dimensional Minkowski space $\R^{1+2}$ to hyperbolic spaces $\H^m$ are globally smooth in time if the initial data is smooth, conditionally on some reasonable claims concerning the local theory of such…

Analysis of PDEs · Mathematics 2009-08-08 Terence Tao

We consider co-rotational wave maps from Minkowski space in $d+1$ dimensions to the $d$-sphere. Recently, Bizo\'n and Biernat found explicit self-similar solutions for each dimension $d\geq 4$. We give a rigorous proof for the mode…

Analysis of PDEs · Mathematics 2016-11-23 Ovidiu Costin , Roland Donninger , Irfan Glogić

We study corotational wave maps from $(1+4)$-dimensional Minkowski space into the $4$-sphere. We prove the stability of an explicitly known self-similar wave map under perturbations that are small in the critical Sobolev space.

Analysis of PDEs · Mathematics 2022-01-28 Roland Donninger , David Wallauch

We consider harmonic maps from Minkowski space into the three sphere. We are especially interested in solutions which are asymptotically constant, i.e. converge to the same value in all directions of spatial infinity. Physical 3-space can…

Astrophysics · Physics 2010-11-19 Lukas Lichtensteiger , Ruth Durrer
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