skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Analytical approximations for spiral waves

Journal Article · · Chaos (Woodbury, N. Y.)
DOI:https://doi.org/10.1063/1.4848576· OSTI ID:22251732
;  [1]
  1. Institut für Theoretische Physik, Technische Universität Berlin, Hardenbergstrasse 36, EW 7-1, 10623 Berlin (Germany)

We propose a non-perturbative attempt to solve the kinematic equations for spiral waves in excitable media. From the eikonal equation for the wave front we derive an implicit analytical relation between rotation frequency Ω and core radius R{sub 0}. For free, rigidly rotating spiral waves our analytical prediction is in good agreement with numerical solutions of the linear eikonal equation not only for very large but also for intermediate and small values of the core radius. An equivalent Ω(R{sub +}) dependence improves the result by Keener and Tyson for spiral waves pinned to a circular defect of radius R{sub +} with Neumann boundaries at the periphery. Simultaneously, analytical approximations for the shape of free and pinned spirals are given. We discuss the reasons why the ansatz fails to correctly describe the dependence of the rotation frequency on the excitability of the medium.

OSTI ID:
22251732
Journal Information:
Chaos (Woodbury, N. Y.), Vol. 23, Issue 4; Other Information: (c) 2013 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 1054-1500
Country of Publication:
United States
Language:
English

Similar Records

Light-induced frequency shift in chemical spirals
Journal Article · Thu Dec 05 00:00:00 EST 1996 · Journal of Physical Chemistry · OSTI ID:22251732

Observational foundations of density-wave models for spiral structure
Journal Article · Fri Sep 01 00:00:00 EDT 1978 · Sov. Astron. AJ (Engl. Transl.); (United States) · OSTI ID:22251732

A CGPS look at the spiral structure of the outer Milky Way. I. Distances and velocities to star-forming regions
Journal Article · Sun Nov 01 00:00:00 EDT 2015 · The Astronomical Journal (Online) · OSTI ID:22251732