00:01
So we're given this hamiltonian, just t plus v.
00:07
It's in three dimensions, so our p represents the three -dimensional moment.
00:12
I'm gonna write it in spherical coordinates because we're already halfway there anyway.
00:21
And my h looks like this.
00:32
But the interesting thing about the potential is that it goes like one over r squared.
00:38
All the terms go like one over r squared.
00:44
So that means that really it's kind of some function of theta divided by r squared.
00:54
That makes it possible to separate the hamilton -jacobi equation.
00:59
So for the principal function, s, we have an equation that looks like this, okay? and if i make the substitution, we make s a sum of terms, each of which is a function of only one variable.
01:38
And substitute that in, we can see how that separation is gonna work, okay? and i'm gonna make an observation right away.
02:14
This is equal to zero.
02:19
So if i make, right away i can see that t and phi are fairly simple.
02:34
I'm gonna call it et.
02:35
In a minute, i'm gonna replace that with minus e times t because written this way, the energy is negative.
02:42
M is the z component of angular momentum, capital m.
02:48
Little m is the mass.
02:53
Here's my theta equation.
03:11
Capital l is the total angular momentum.
03:22
Then my radial equation looks like this.
03:27
So then i gotta put in the negative e.
03:30
And i can see why i wanna do that.
03:32
If i look at the radial equation, these two terms over here are always positive...