In the simplest case,
$\frac{dx}{dt} = f(x)$
where $f$ has no explicit time dependance.
Consider $f(x) = sin(x)$. For this, the solution fo the diff eq is
Which is a pain to evaluate, and does not give much insight.
We can also represent the differential equation to be a vector field, which tells us the velocity vector on a line.
Define
$\eta(n) = x(t) - x^*$ as a perturbation around $x^*$
Then, $\dot \eta = f(x) - 0$
But, $f(x) = f(x^* + \eta) = f(x^*) + \eta f’(x^*) + \mathcal{O}(\eta^2)$
But $f(x^*) = 0$, and $f(x) = \dot \eta$
Hence,
\[\dot \eta = \eta f'(x^\*)\]Which has a solution
$\eta = \eta_0 \exp(f’(x^*) t)$.
Hence the fixed point is
$\begin{cases}
\text{Stable} & f’(x^) < 0
\text{Unstable}&f’(x^) > 0
\text{Non linear analysis necessary}&f’(x^*)=0
\end{cases}$
$\tau = \frac{1}{\vert f’(x^*)\vert}$
Fixed points are $N = 0$ (unstable) and $N = k$ (stable)
The flow accelerates from $0$ till $K/2$, then decelerates till $K$ and then stops.
$Q^*= V_0C$
Consider $\dot x = x^2 + 1$. With $x(0) = 0$, the solution is $x = tan(t)$ which exists only in $t\in(-\pi/2, \pi/2)$.
Therefore, the system blows up to infinity in finite time.
For a vector field on a line,
If $b\dot x\gg m\ddot x$,
\[\dot x = F(x)/b\]which is a flow on a single line.
As in previous section, $f(x)$ can be considered as a “force” on a particle, but the particle is highly damped (think: in a highly viscous fluid).
Hence, plotting $F(x)$ tells us a “mountain” to ascend or descend.
While the maps are simple, We can still get bifurcations by varying some parameter.
Bifurcations can either be points where
See [2022-01-18#Bifurcations] for more.
Consider
\[\dot x = x^2 + r\]Here, we see a saddlenode bifurcation, or tangent bifurcation at $r = 0$
This is very similar to [2022-02-01#Tangent Bifurcation].
The trick is to plot $r-x$ and $e^{-x}$, and to see for what value of $r$ it intersects.
Since intersection must be tangential, $\frac{d(r_c-x)}{dx} = \frac{d e^{-x}}{dx}$ at point of intersection $x^*$
Hence, $e^{x^*} = 1$ is the point of intersection. That is, $x^* = 0$.
But also, $r_c-x^* = e^{-x^*}$, which implies $r_c = 1$
For tangent bifurcations, $f(x, r)$ generally looks like $r \pm x^2$. This comes from the taylor expansion and that $f = 0$ and $f’ = 0$ at $(x^*, r_c)$.
Now consider a Normal form of type
\[f(x) = rx - x^2 = x(r-x)\]In this case, the $\dot x$ vs $x$ plot moves horizontally and vertically.
From linear stability analysis,
$f’(x, r) = r - 2x$ implies
To get to a normal mode, we can take taylor expansion of $f$ and then make a change of variable to bring it to the form $\dot x = rx-x^2$. From there, $r=0$ is the point of transcritical bifurcation, as $x^*=0$ is always a solution.
The normal mode is of the form
\[\dot x = rx-x^3\]However, at $r=0$, linearity vanishes, but $x^* = 0$ is still weakly stable, in that perturbations do not decay exponentially fast, but only algebraically fast. This is known as Critical Slowing down
These are also called second order phase transitions.
However, this is rare in physical systems and there’s not much to see in this system. Hence, we add a -ve term
\[\dot x = rx + x^3 -x^5\]gives a saddlenode bifurcation for $\vert x^*\vert \gg 0$