Thomas' cyclically symmetric attractor

From Infogalactic: the planetary knowledge core
Jump to: navigation, search
File:Thomas' cyclically symmetric attractor.png
Thomas' cyclically symmetric attractor.

In the dynamical systems theory, Thomas' cyclically symmetric attractor is a 3D strange attractor originally proposed by René Thomas.[1] It has a simple form which is cyclically symmetric in the x,y, and z variables and can be viewed as the trajectory of a frictionally dampened particle moving in a 3D lattice of forces.[2] The simple form has made it a popular example.

It is described by the differential equations

\frac{dx}{dt} = \sin(y)-bx
\frac{dy}{dt} = \sin(z)-by
\frac{dz}{dt} = \sin(x)-bz

where b is a constant.

b corresponds to how dissipative the system is, and acts as a bifurcation parameter. For b>1 the origin is the single stable equilibrium. At b=1 it undergoes a pitchfork bifurcation, splitting into two attractive fixed points. As the parameter is decreased further they undergo a Hopf bifurcation at b\approx 0.32899, creating a stable limit cycle. The limit cycle the undergoes a period doubling cascade and becomes chaotic at b\approx 0.208186. Beyond this the attractor expands, undergoing a series of crises (up to six separate attractors can coexist for certain values). The fractal dimension of the attractor increases towards 3.[2]

In the limit b=0 the system lacks dissipation and the trajectory ergodically wanders the entire space (with an exception for 1.67%, where it drifts parallel to one of the coordinate axes: this corresponds to quasiperiodic torii). The dynamics has been described as deterministic fractional Brownian motion, and exhibits anomalous diffusion.[2][3]

References

  1. Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. Lua error in package.lua at line 80: module 'strict' not found.