Saddle-node bifurcation explained

In the mathematical area of bifurcation theory a saddle-node bifurcation, tangential bifurcation or fold bifurcation is a local bifurcation in which two fixed points (or equilibria) of a dynamical 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 sky 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).

Saddle-node bifurcations may be associated with hysteresis loops and catastrophes.

Normal form

A typical example of a differential equation with a saddle-node bifurcation is:

dx
dt

=r+x2.

Here

x

is the state variable and

r

is the bifurcation parameter.

r<0

there are two equilibrium points, a stable equilibrium point at

-\sqrt{-r}

and an unstable one at

+\sqrt{-r}

.

r=0

(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.

r>0

there are no equilibrium points.

In fact, this is a normal form of a saddle-node bifurcation. A scalar differential equation

\tfrac{dx}{dt}=f(r,x)

which has a fixed point at

x=0

for

r=0

with

\tfrac{\partialf}{\partialx}(0,0)=0

is locally topologically equivalent to
dx
dt

=r\pmx2

, provided it satisfies

\tfrac{\partial2f}{\partialx2}(0,0)\ne0

and

\tfrac{\partialf}{\partialr}(0,0)\ne0

. The first condition is the nondegeneracy condition and the second condition is the transversality condition.

Example in two dimensions

An example of a saddle-node bifurcation in two dimensions occurs in the two-dimensional dynamical system:

dx
dt

=\alpha-x2

dy
dt

=-y.

As can be seen by the animation obtained by plotting phase portraits by varying the parameter

\alpha

,

\alpha

is negative, there are no equilibrium points.

\alpha=0

, there is a saddle-node point.

\alpha

is positive, there are two equilibrium points: that is, one saddle point and one node (either an attractor or a repellor).

Other examples are in modelling biological switches.[1] Recently, it was shown that under certain conditions, the Einstein field equations of General Relativity have the same form as a fold bifurcation.[2] A non-autonomous version of the saddle-node bifurcation (i.e. the parameter is time-dependent) has also been studied.[3]

See also

References

Notes and References

  1. Chong . Ket Hing . Samarasinghe . Sandhya . Kulasiri . Don . Zheng . Jie . 2015 . Computational techniques in mathematical modelling of biological switches . 21st International Congress on Modelling and Simulation . 10220/42793 .
  2. 10.1016/j.geomphys.2017.10.001 . Einstein's field equations as a fold bifurcation . Journal of Geometry and Physics . 123 . 434–7 . 2018 . Kohli . Ikjyot Singh . Haslam . Michael C . 1607.05300 . 2018JGP...123..434K . 119196982 .
  3. Li. Jeremiah H.. Ye. Felix X. -F.. Qian. Hong. Huang. Sui. 2019-08-01. Time-dependent saddle–node bifurcation: Breaking time and the point of no return in a non-autonomous model of critical transitions. Physica D: Nonlinear Phenomena. 395. 7–14. 10.1016/j.physd.2019.02.005. 31700198 . 6836434 . 0167-2789. 1611.09542. 2019PhyD..395....7L .