- Saddle-node bifurcation
In the mathematical area of
bifurcation theory a saddle-node bifurcation or tangential bifurcation is alocal bifurcation in which twofixed point s (or equilibria) of adynamical system collide and annihilate each other. The term 'saddle-node bifurcation' is most often used in reference to continuous dynamical systems. In discrete dynamical systems, the same bifurcation is often instead called a fold bifurcation. Another name is blue skies bifurcation in reference to the sudden creation of two fixed points.If the phase space is one-dimensional, one of the equilibrium points is unstable (the saddle), while the other is stable (the node).
The normal form of a saddle-node bifurcation is:
::
Here is the state variable and is the bifurcation parameter.
*If there are two equilibrium points, a stable equilibrium point at and an unstable one at .
*At (the bifurcation point) there is exactly one equilibrium point. At this point the fixed point is no longer hyperbolic. In this case the fixed point is called a saddle-node fixed point.
*If there are no equilibrium points.A saddle-node bifurcation occurs in the consumer equation (see
transcritical bifurcation ) if the consumption term is changed from to , that is the consumption rate is constant and not in proportion to resource .Saddle-node bifurcations may be associated with hysteresis loops and catastrophes.
Example
An example of a saddle-node bifurcation in two-dimensions occurs in the two-dimensional dynamical system:
:
:As can be seen by the animation obtained by plotting phase portraits by varying the parameter ,
* When is negative, there are no equilibrium points.
* When , there is a saddle-node point.
* When is positive, there are two equilibrium points: that is, onesaddle point and one node (either an attractor or a repellor),.See also
*
Pitchfork bifurcation *
Transcritical bifurcation *
Hopf bifurcation
*Saddle point
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