Chem 3240 · Lecture 3.7

\Psi_n(x,t) = \psi_n(x)\,e^{-iE_nt/\hbar} \qquad\Longrightarrow\qquad \lvert\Psi_n\rvert^2 = \lvert\psi_n\rvert^2 \ \text{ never moves}

\lvert\Psi\rvert^2 = \tfrac{1}{2}\big(\psi_1^2 + \psi_2^2\big) + \psi_1\psi_2\cos\omega t, \qquad \omega = \frac{E_2 - E_1}{\hbar}
\Psi(x,0) = \sum_n c_n\,\psi_n(x) \quad\Longrightarrow\quad \Psi(x,t) = \sum_n c_n\,e^{-iE_nt/\hbar}\,\psi_n(x)
Show that \Psi(x,t) = \sum_n c_n\,e^{-iE_nt/\hbar}\,\psi_n(x) satisfies i\hbar\,\partial\Psi/\partial t = \hat{H}\Psi.
i\hbar\,\frac{\partial\Psi}{\partial t} = \sum_n c_n\,i\hbar\left(-\frac{iE_n}{\hbar}\right)e^{-iE_nt/\hbar}\,\psi_n = \sum_n c_n\,E_n\,e^{-iE_nt/\hbar}\,\psi_n
\hat{H}\Psi = \sum_n c_n\,e^{-iE_nt/\hbar}\,\hat{H}\psi_n = \sum_n c_n\,E_n\,e^{-iE_nt/\hbar}\,\psi_n \quad\checkmark
Term by term, using \hat{H}\psi_n = E_n\psi_n. At t = 0 every phase is 1.

# the grid and D2 of Lecture 3.5; spring with hbar = m = omega = 1; a packet pulled to x = 3
H = -0.5 * D2 + np.diag(0.5 * x**2)
psi0 = np.exp(-(x - 3)**2 / 2) / np.pi**0.25
E, phi = np.linalg.eigh(H); phi /= np.sqrt(dx) # 1. diagonalize once: E_n and psi_n
c = phi.T @ psi0 * dx # 2. expand: c_n = <psi_n|Psi(0)>
psi_t = phi @ (c * np.exp(-1j * E * t)) # 3. attach the phases, add up: Psi(x, t)
1. The weights. Each c_n turns like a clock hand; its length stays:
\lvert c_n\,e^{-iE_nt/\hbar}\rvert^2 = \lvert c_n\rvert^2
2. The normalization. The cross terms die by orthogonality, \langle \psi_m \vert \psi_n \rangle = \delta_{mn}:
\langle \Psi(t) \vert \Psi(t) \rangle = \sum_m\sum_n c_m^*\,c_n\,e^{i(E_m - E_n)t/\hbar}\,\langle \psi_m \vert \psi_n \rangle = \sum_n \lvert c_n\rvert^2 = 1
Take the time derivative of \langle A\rangle = \langle\Psi\vert\hat{A}\vert\Psi\rangle, and plug in the Schrödinger equation for the ket and the bra:
\partial_t\lvert\Psi\rangle = \frac{1}{i\hbar}\,\hat{H}\lvert\Psi\rangle \qquad\qquad \partial_t\langle\Psi\rvert = -\frac{1}{i\hbar}\,\langle\Psi\rvert\hat{H}
\frac{d}{dt}\langle A\rangle = \frac{i}{\hbar}\,\big\langle[\hat{H},\hat{A}]\big\rangle \qquad (\hat{A} \text{ not explicitly time dependent})
\hat{H} = \frac{\hat{p}^2}{2m} + V(x)
| observable | [\hat{H}, \cdot\,] | conserved when |
|---|---|---|
| energy \hat{H} | 0 | always |
| momentum \hat{p} | i\hbar\,dV/dx | no force |
| position \hat{x} | -i\hbar\,\hat{p}/m | only while \langle p\rangle = 0 |
With V = 0, \hat{H} = \hat{p}^2/2m. Is e^{ipx/\hbar} an eigenfunction of \hat{p}? Of \hat{H}? Of \hat{x}?
\hat{p}\,e^{ipx/\hbar} = -i\hbar\,\frac{d}{dx}\,e^{ipx/\hbar} = p\,e^{ipx/\hbar} \qquad \text{yes: eigenvalue } p
\hat{H}\,e^{ipx/\hbar} = \frac{\hat{p}^2}{2m}\,e^{ipx/\hbar} = \frac{p^2}{2m}\,e^{ipx/\hbar} \qquad \text{yes: eigenvalue } E_p = \frac{p^2}{2m}
\hat{x}\,e^{ipx/\hbar} = x\,e^{ipx/\hbar} \qquad \text{no: } x \text{ is a function, not a number}
\Psi(x,t) = \int \phi(p)\,\frac{e^{i(px - E_pt)/\hbar}}{\sqrt{2\pi\hbar}}\,dp

\frac{d\langle x\rangle}{dt} = \frac{\langle p\rangle}{m} \qquad\qquad \frac{d\langle p\rangle}{dt} = -\Big\langle\frac{dV}{dx}\Big\rangle

\langle x\rangle(t) = \sum_n \lvert c_n\rvert^2 x_{nn} + \sum_{n\neq m} c_m^*\,c_n\,x_{mn}\,e^{-i(E_n - E_m)t/\hbar}, \qquad x_{mn} = \langle\psi_m\vert\hat{x}\vert\psi_n\rangle

\frac{1}{2}\psi_1 + \frac{1}{2}\psi_2 + \frac{1}{\sqrt{2}}\psi_3 in a box: which of \omega_{21}, \omega_{32}, \omega_{31} appear in \langle x\rangle(t)?
About the center, \psi_1 and \psi_3 are even, x - L/2 is odd:
x_{13} = \tfrac{L}{2}\int\psi_1\psi_3\,dx + \int\psi_1\big(x - \tfrac{L}{2}\big)\psi_3\,dx = 0 + 0
\omega_{21} = 3E_1/\hbar and \omega_{32} = 5E_1/\hbar appear; \omega_{31} = 8E_1/\hbar does not. A selection rule.

T_{\text{rev}} = \frac{2\pi\hbar}{E_1} = \frac{4mL^2}{\pi\hbar}
How long does an electron in a box 1 nm long take to rebuild any starting state?
T_{\text{rev}} = \frac{4\,(9.109\times10^{-31}\ \text{kg})\,(10^{-9}\ \text{m})^2}{\pi\,(1.055\times10^{-34}\ \text{J s})} = 1.1\times10^{-14}\ \text{s} = 11\ \text{fs}
Twice the box, four times slower: T_{\text{rev}} \propto L^2.


| postulate | in equations | |
|---|---|---|
| 1 | the state is a normalized wavefunction | \langle \psi \vert \psi \rangle = 1 |
| 2 | observables are linear Hermitian operators | \hat{A} = \hat{A}^\dagger, \hat{A}\phi_n = a_n\phi_n |
| 3 | a reading is an eigenvalue; the state becomes its eigenfunction | a_n, then \psi \to \phi_n |
| 4 | probabilities and averages | p_n = \lvert\langle \phi_n \vert \psi \rangle\rvert^2, \langle A\rangle = \langle \psi \vert \hat{A} \vert \psi \rangle |
| 5 | evolution by the Schrödinger equation | \Psi(t) = \sum_n c_n e^{-iE_nt/\hbar}\psi_n |
Diagonalize \hat{H} once, and any state’s future follows: expand, attach to each eigenstate its phase e^{-iE_nt/\hbar}, add up. The energy probabilities and the norm never change; the relative phases make all the motion, at the Bohr frequencies (E_n - E_m)/\hbar that spectroscopy measures. Averages obey Newton’s laws, exactly so in a harmonic well, and observables that commute with \hat{H} are conserved.
Chem 3240 · Quantum Mechanics