Solution (source code)

= Solution

<Ehrenfest theorem> relates the dynamics of quantum <expectation values> to operator <commutators>. For a normalized state obeying $i\hbar|\dot\psi\rangle=\widehat H|\psi\rangle$ and a possibly time-dependent <observable> $\widehat A$, differentiate $\langle A\rangle=\langle\psi|\widehat A|\psi\rangle$. Using the adjoint <Schrödinger equation> for the bra gives
$$
\begin{aligned}
\frac d{dt}\langle A\rangle
&=\frac i\hbar\langle HA\rangle-\frac i\hbar\langle AH\rangle
+\left\langle\frac{\partial A}{\partial t}\right\rangle\\
&=\frac1{i\hbar}\langle[A,H]\rangle
+\left\langle\frac{\partial A}{\partial t}\right\rangle.
\end{aligned}
$$
Thus
$$
\boxed{\frac d{dt}\langle A\rangle=
\frac1{i\hbar}\langle[A,H]\rangle+\langle\partial_t A\rangle.}
$$
The identity assumes a common domain on which the required products and <derivatives> are defined.

For $H=p^2/(2m)+V(x)$, the <canonical commutation relation> gives $[x,H]=i\hbar p/m$ and $[p,H]=-i\hbar V'(x)$. Therefore
$$
\boxed{\frac d{dt}\langle x\rangle=\frac{\langle p\rangle}{m},\qquad
\frac d{dt}\langle p\rangle=-\langle V'(x)\rangle.}
$$
These resemble <Hamilton's equations> and <Newton's second law>, but generally $\langle V'(x)\rangle\ne V'(\langle x\rangle)$. If the state is localized about $\overline x=\langle x\rangle$, a local expansion gives
$$
\langle V'(x)\rangle=V'(\overline x)+\frac12V^{(3)}(\overline x)
\langle(x-\overline x)^2\rangle+\cdots.
$$
The classical trajectory equation for the mean is accurate when the force changes little across the <wave packet>. For a quadratic <harmonic potential>, $V'$ is linear and this closure is exact for every state with the relevant finite moments: $m\,d^2\langle x\rangle/dt^2=-m\omega^2\langle x\rangle$. This exact classical evolution of the centroid does not eliminate its quantum <position uncertainty> or make every state a point particle.

The <correspondence principle> is broader: quantum predictions recover classical ones in an appropriate limit, such as large action compared with $\hbar$ and observations that cannot resolve individual quantum levels. It is not the assertion that every large <quantum number> automatically makes every possible state classical. Delocalized superpositions and interference can remain significant unless the physical preparation and measurement justify a classical description.

A spectral example is useful. For a <quantum harmonic oscillator>, neighboring levels differ by $\hbar\omega$, giving transition <frequency> $\omega/(2\pi)$, equal to its classical oscillation <frequency>. A <coherent state> makes the connection more concrete: its mean <position> and <momentum> oscillate classically while the finite-width Gaussian profile retains its quantum uncertainty. For hydrogenic Bohr levels $E_n=-A/n^2$, transitions between nearby large $n$ have $\Delta E/\hbar\simeq2A/(\hbar n^3)$, which equals the classical circular orbital angular <frequency> in that model. \b[Ehrenfest's theorem supplies an exact expectation-value bridge; a classical trajectory follows only when the force can also be evaluated at the mean <position>.]