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Saddle-node

 

In a saddle-node bifurcation  a pair of periodic orbits are created ``out of nothing.'' One of the periodic orbits is always unstable (the saddle), while the other periodic orbit is always stable (the node). The basic bifurcation diagram for a saddle-node bifurcation looks like that shown in Figure 2.15.

  
Figure 2.15: Saddle-node bifurcation diagram.

The saddle-node bifurcation is fundamental to the study of nonlinear systems since it is one of the most basic processes by which periodic orbits are created.

A saddle-node bifurcation is also referred to as a tangent bifurcation  because of the mechanism by which the orbits are born. Consider the nth composite of some mapping function tex2html_wrap_inline12213 which is near to a tangency with the line y = x.

  
Figure 2.16: Tangency mechanism for a saddle-node bifurcation.

Let tex2html_wrap_inline12408 be the value at which a saddle-node bifurcation occurs. Notice in Figure 2.16 that tex2html_wrap_inline12223 is tangent to the line y = x at tex2html_wrap_inline12408 . For tex2html_wrap_inline12416 , no period n orbits exist in this neighborhood, but for tex2html_wrap_inline12420 two orbits are born. The local stability of a point of a map is determined by tex2html_wrap_inline12422 . Since tex2html_wrap_inline12424 is tangent to y = x at a bifurcation, it follows that at tex2html_wrap_inline12408 ,gif

  equation1673

Tangent bifurcations abound in the quadratic map. For instance, a pair of period three orbits are created by a tangent bifurcation in the quadratic map when tex2html_wrap_inline12430 . As illustrated in Figure 2.17

  
Figure 2.17: A pair of period three orbits created by a tangent bifurcation in the quadratic map (shown with the unstable period one orbits).

for tex2html_wrap_inline12432 , there are eight points of intersection. Two of the intersection points belong to the period one orbits, while the remaining six make up a pair of period three orbits. Near to tangency, the absolute value of the slope at three of these points is greater than one--this is the unstable period three orbit. The remaining three points form the stable periodic orbit. The birth of this stable period three orbit is clearly visible as the period three window in our numerically constructed bifurcation diagram of the quadratic map, Figure 2.14. In fact, all the odd-period orbits of the quadratic map are created by some sort of tangent bifurcation.


next up previous contents
Next: Period Doubling Up: Local Bifurcation Theory Previous: Local Bifurcation Theory

Nicholas B. Tufillaro
Mon Mar 3 01:58:02 PST 1997