Neither Example 4.4 nor Problem 4.73 actually solved the Schrödinger equation for the Stern–Gerlach experiment. In this problem we will see how to set up that calculation. The Hamiltonian for a neutral, spin 1/2 particle traveling through a Stern–Gerlach device is
H=\frac{p^{2}}{2 m}-\gamma B \cdot S .
where B is given by Equation 4.169. The most general wave function for a spin- particle—including both spatial and spin degrees of freedom—is
B (x, y, z)=-\alpha x \hat{\imath}+\left(B_{0}+\alpha z\right) \hat{k} (4.169).
\Psi( r , t)=\Psi_{+}( r , t) \chi_{+}+\Psi_{-}( r , t) \chi_{-} .
(a) Put \Psi ( r , t) into the Schrödinger equation
H \Psi=i \hbar \frac{\partial}{\partial t} \Psi .
to obtain a pair of coupled equations for \Psi_{\pm} . Partial answer:
-\frac{\hbar^{2}}{2 m} \nabla^{2} \Psi_{+}-\frac{\hbar}{2} \gamma\left(B_{0}+\alpha z\right) \Psi_{+}+\frac{\hbar}{2} \gamma \alpha x \Psi_{-}=i \hbar \frac{\partial}{\partial t} \Psi_{+} .
(b) We know from Example 4.3 that the spin will precess in a uniform field B_{0} \hat{k} . We can factor this behavior out of our solution—with no loss of generality—by writing
\Psi_{\pm}( r , t)=e^{\pm i \gamma B_{0} t / 2} \tilde{\Psi}( r , t) .
Find the coupled equations for \tilde{\Psi}_{\pm} . Partial answer:
-\frac{\hbar^{2}}{2 m} \nabla^{2} \tilde{\Psi}_{+}-\frac{\hbar}{2} \gamma \alpha z \tilde{\Psi}_{+}+\frac{\hbar}{2} \gamma \alpha x e^{-i \gamma B_{0} t} \tilde{\Psi}_{-}=i \hbar \frac{\partial}{\partial t} \tilde{\Psi}_{+} .
(c) If one ignores the oscillatory term in the solution to (b)—on the grounds that it averages to zero (see discussion in Example 4.4)—one obtains uncoupled equations of the form
-\frac{\hbar^{2}}{2 m} \nabla^{2} \tilde{\Psi}_{\pm}+V_{\pm} \tilde{\Psi}_{\pm}=i \hbar \frac{\partial}{\partial t} \tilde{\Psi}_{\pm} .
Based upon the motion you would expect for a particle in the “potential” V_{\pm} , explain the Stern–Gerlach experiment.