00:01
Okay, so we're given this hamiltonian, that's our classical hamiltonian.
00:04
We want to construct the schrodinger equation, and what we want is the time dependent schrodinger equation, because our next step is going to be to look at the probability current, and for that we need the time dependent equation.
00:20
So we know that where h is written as an operator, and for that we have to basically replace the momenta by derivatives, and that's all hitting on the function phi, psi.
01:22
Okay, so let's expand this out a little bit.
01:37
So first of all, we get what's essentially a laplacian.
01:47
I'm going to write them out with the psi's.
01:50
Those come from this partial x squared term, and the partial y squared term, and the partial z squared term, and then we got terms that are proportional to just the first derivatives, and those look like this, and then we get the so -called quadratic terms.
02:51
That's our schrodinger equation.
02:57
So then to do the conservation law, we want to look at the probability current, or figure out what it is.
03:04
So rho is psi, psi, psi.
03:09
That's the probability distribution...