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Time evolution of the state vector

The time evolution of the state vector is prescribed by the Schrödinger equation

\begin{displaymath}
i\hbar {\partial \over \partial t} \vert\Psi(t)\rangle = H\vert\Psi(t)\rangle
\end{displaymath}

where $H$ is the Hamiltonian operator. This equation can be solved, in principle, yielding

\begin{displaymath}
\vert\Psi(t)\rangle = e^{-iHt/\hbar}\vert\Psi(0)\rangle
\end{displaymath}

where $\vert\Psi(0)\rangle $ is the initial state vector. The operator

\begin{displaymath}
U(t) = e^{-iHt\hbar}
\end{displaymath}

is the time evolution operator or quantum propagator. Let us introduce the eigenvalues and eigenvectors of the Hamiltonian $H$ that satisfy

\begin{displaymath}
H\vert E_i\rangle = E_i \vert E_i\rangle
\end{displaymath}

The eigenvectors for an orthonormal basis on the Hilbert space and therefore, the state vector can be expanded in them according to

\begin{displaymath}
\vert\Psi(t)\rangle = \sum_i c_i(t) \vert E_i\rangle
\end{displaymath}

where, of course, $c_i(t) = \langle E_i\vert\Psi(t)\rangle $, which is the amplitude for obtaining the value $E_i$ at time $t$ if a measurement of $H$ is performed. Using this expansion, it is straightforward to show that the time evolution of the state vector can be written as an expansion:
$\displaystyle \vert\Psi(t)\rangle$ $\textstyle =$ $\displaystyle e^{-iHt\hbar}\vert\Psi(0)\rangle$  
  $\textstyle =$ $\displaystyle e^{-iHt/\hbar}\sum_i\vert E_i\rangle \langle E_i\vert\Psi(0)\rangle$  
  $\textstyle =$ $\displaystyle \sum_i e^{-iE_i t/\hbar}\vert E_i\rangle \langle E_i\vert\Psi(0)\rangle$  

Thus, we need to compute all the initial amplitudes for obtaining the different eigenvalues $E_i$ of $H$, apply to each the factor $\exp(-iE_it/\hbar)\vert E_i\rangle $ and then sum over all the eigenstates to obtain the state vector at time $t$.

If the Hamiltonian is obtained from a classical Hamiltonian $H(x,p)$, then, using the formula from the previous section for the action of an arbitrary operator $A(X,P)$ on the state vector in the coordinate basis, we can recast the Schrödiner equation as a partial differential equation. By multiplying both sides of the Schrödinger equation by $\langle x\vert$, we obtain

$\displaystyle \langle x\vert H(X,P)\vert\Psi(t)\rangle$ $\textstyle =$ $\displaystyle i\hbar {\partial \over \partial t}\langle x\vert\Psi(t)\rangle$  
$\displaystyle H\left(x,{\hbar \over i}{\partial \over \partial x}\right)\Psi(x,t)$ $\textstyle =$ $\displaystyle i\hbar {\partial \over \partial t}\Psi(x,t)$  

If the classical Hamiltonian takes the form

\begin{displaymath}
H(x,p) = {p^2 \over 2m} + U(x)
\end{displaymath}

then the Schrödinger equation becomes

\begin{displaymath}
\left[-{\hbar^2 \over 2m}{\partial^2 \over \partial x^2} + U(x)\right]\Psi(x,t)
= i\hbar {\partial \over \partial t}\Psi(x,t)
\end{displaymath}

which is known as the Schrödinger wave equation or the time-dependent Schrödinger equation.

In a similar manner, the eigenvalue equation for $H$ can be expressed as a differential equation by projecting it into the $X$ basis:

$\displaystyle \langle x\vert H\vert E_i\rangle$ $\textstyle =$ $\displaystyle E_i \langle x\vert E_i\rangle$  
$\displaystyle H\left(x,{\hbar \over i}{\partial \over \partial x}\right)\psi_i(x)$ $\textstyle =$ $\displaystyle E_i \psi_i(x)$  
$\displaystyle \left[-{\hbar^2 \over 2m}{\partial^2 \over \partial x^2} + U(x)\right]\psi_i(x)$ $\textstyle =$ $\displaystyle E_i \psi_i(x)$  

where $\psi_i(x) = \langle x\vert E_i\rangle $ is an eigenfunction of the Hamiltonian.


next up previous
Next: The Heisenberg uncertainty principle Up: The fundamental postulates of Previous: Measurement
Mark E. Tuckerman 2008-03-15