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Let us restate the problem for ease of reference. The equations are

$\dot{x}(t)=y(t)$
$\dot{y}(t)= - 4 x(t) + y(t)^2$

Physically they describe an anharmonic oscillator with spatial coordinate $x(t)$ and velocity $y(t)$ in the potential

$U = 2 x^2 - \frac{1}{3} x^3$

and the energy

$E = \frac{1}{2} y^2 + U(x)$

The problem is then: given two solutions

$s1(t) = (x1(t), y1(t))$
$s2(t) = (x2(t), y2(t))$

corresponding to the initial conditions

$s1(0) = (x1(t=0) = x10, y1(t=0) = y10)$ $s2(0) = (x2(t=0) = x20, y2(t=0) = y20)$

Assuming that $y10$ and $y20$ do not vanish show that the quantity

$d(t) = y1(t) + y2(t)$

becomes $\neq 0$ for times $t>0$ even if it is $= 0$ for $t = 0$, i.e.

$y10 + y20 = 0$.

We proceed by expanding the solution $y(t)$ into a power series in t.

$y(t) = y(0) + t \dot{y}(0) + \frac{1}{2} \ddot{y}(0) + \frac{1}{3} \frac{\partial ^3y(0)}{\partial t^3} + ...$

In order to have $d(t) = 0$, all coefficients must vanish. These can be expressed through the initial values, and the first coefficients are

$c(0) = (y10 + y20) $
$c(1) = - 4 (x10 + x20) + (x10^2 + x20^2) $
$c(2) = - 4 (y10 + y20) + 2 ( x10 y10 + x20 y20 ) $
$c(3) = 2 (y10^2 + y20^2) + 2 ( x10^3+x20^3 ) -12 (x10^2 + x20^2) + 16 (x10 + x20)) $

Since we have $y10 + y20 = 0$, $d(t) = 0$ requires

$0 = - 4 (x10+ x20) + (x10^2 + x20^2) $

On the other hand, for $d(t) = 0$ to hold for arbitrary long times the period of motion for $s1$ and $s2$ must be the same. This in turn requires the energy $E$ to be the same, which means

$0 = (6 x10^2- x10^3)-(6 x20^2- x20^3) $

These two equations for $x10$ and $x20$ have the solutions

$sol1 = (x10 = x20 = 0)$
$sol2 = (x10 = x20 = 4)$

The orbits obey the equation

$\frac{d y}{d x}=\frac{y^2-4 x}{y}$

Multiplying by $y$ this can be written as

$\frac{1}{2}\frac{d y^2}{\text{dx}}=y^2-4 x$

and is easily integrated to give

$y^2=c \exp (2 x)+4 x+2$

where $c$ is a constant of integration.

If the initial state is $( x(0) = x0$, $y(0) = y0 )$

then

$c=\left(-4 x0+y0^2-2\right) \exp (- 2 \text{x0})$

and the orbit corresponding to this Initial state is

$y^2=\left(-4 \text{x0}+\text{y0}^2-2\right) \exp (2 (x-\text{x0}))+4 x+2$

Now the sign of the factor in front of the exponential

$s=\left(-4 \text{x0}+\text{y0}^2-2\right)$

defines distinguishes between finite ($s<0$) and unbounded ($s>0$) orbits. We therefore call the orbit $s=0$ the separatrix.

Second integration, time dependence, frequency of oscillation

Because of

$dx/dt = y[x] = Sqrt[2 + 4 x + c Exp[2 x]]$

variables can be separated an we get the time $t$ as a function of $x$:

$t=\int_{\text{x0}}^x \frac{1}{\sqrt{c \exp (2 z)+4 z+2}} \, dz+\text{t0}$