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Schödinger's Equation

According to the fourth postulate of quantum mechanics, the time evolution of the state function $\psi(x,t)$ is determined by the so-called time dependent Schrödinger's equation:

\begin{displaymath}
i\hbar \frac{\partial}{\partial t} \psi({\bf x},t) = H\psi({\bf x},t).
\end{displaymath} (1)

The operator $H$ is the Hamiltonian of the system. If $H$ is time-independent, we can separate this equatioon into spatial and time-dependent components:
\begin{displaymath}
\psi({\bf x},t) = \phi({\bf x})\chi(t).
\end{displaymath} (2)

By substituting into (1), we obtain:
\begin{displaymath}
i\hbar\frac{\partial \chi/t}{\chi}=\frac{H\phi}{\phi}.
\end{displaymath} (3)

This equation is satisfied if both sides are equal to a constant, that we call $E$:
$\displaystyle H\phi({\bf x}) = \phi({\bf x})$     (4)
$\displaystyle (\frac{\partial}{\partial t} + \frac{iE}{\hbar}) \chi(t) = 0$     (5)

The first of these equations is the time-independent or stationary Schödinger's equation. As we can see, $E$ is an eigenvalue of $H$, and therefore we conclude that $E$ is the energy of the system.

The second equation is simply solved to give us the oscillating form

\begin{displaymath}
\chi(t)=A\exp{(\frac{-iEt}{\hbar})}
\end{displaymath} (6)

Suppose that we solve the time-independent Schödinger's equation and obtain the eigenvalues and eigenfunctions

\begin{displaymath}
H\phi_n=E_n\phi_n,
\end{displaymath} (7)

For each such solution there is a corresponding solution to the time-dependent Schödinger's equation
\begin{displaymath}
\psi_n({\bf x},t) = A\phi_n({\bf x})\exp{(-\frac{iE_nt}{\hbar})}.
\end{displaymath} (8)

In cases with a discrete set of solutions, such as in a finite system, the subindex $n$ is an integer. In cases where one obtains a continuum of solutions, we typically use the letter $k$. For instance, in the case of a free particle in one dimension we have:
\begin{displaymath}
H=\frac{p^2}{2m}=-\frac{\hbar^2}{2m}\nabla^2.
\end{displaymath} (9)

The time-independent Schrödinger's solution becomes
\begin{displaymath}
-\frac{\hbar^2}{2m}\frac{\partial^2}{\partial x^2}\phi(x)=E\phi(x).
\end{displaymath} (10)

The corresponding free-particle solutions are given by
\begin{displaymath}
\phi_k(x)=A\exp(ikx),
\end{displaymath} (11)

with eigenvalue (energy)
\begin{displaymath}
E_k=\frac{\hbar^2k^2}{2m}=\frac{p^2}{2m},
\end{displaymath} (12)

where the momentum of the particle is $p=\hbar^2k^2$.

The solution to the time-dependent Schrödinger's equation will be given by

\begin{displaymath}
\phi_k(x,t)=A\exp{i(kx-\omega t)},
\end{displaymath} (13)

where we have labeled
\begin{displaymath}
\hbar\omega = E_k.
\end{displaymath} (14)


next up previous
Next: Variational Methods Up: Phys 5870: Modern Computational Previous: Phys 5870: Modern Computational
Adrian E. Feiguin 2009-11-04