Wave maps on a wormhole

Piotr Bizoń and Michał Kahl
Phys. Rev. D 91, 065003 – Published 2 March 2015

Abstract

We consider equivariant wave maps from a fixed wormhole spacetime into the 3-sphere. This toy model is designed for gaining insight into the dissipation-by-dispersion phenomena, in particular the soliton resolution conjecture. We first prove that for each topological degree of the map there exists a unique static solution (harmonic map) that is linearly stable. Then, using the hyperboloidal formulation of the initial value problem, we give numerical evidence that every solution starting from smooth initial data of any topological degree evolves asymptotically to the harmonic map of the same degree. The late-time asymptotics of this relaxation process is described in detail.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
1 More
  • Received 17 December 2014

DOI:https://doi.org/10.1103/PhysRevD.91.065003

© 2015 American Physical Society

Authors & Affiliations

Piotr Bizoń1,2 and Michał Kahl1

  • 1Institute of Physics, Jagiellonian University, Kraków, Poland
  • 2Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Golm, Germany

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 91, Iss. 6 — 15 March 2015

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×