Q2 was never assumed, and the practitioners know it is by far the weakest and notoriously misinterpreted paragraph in von Neumann's basic book on foundational QM, ritually, and virtually comically.
His acolyte H Groenewold resolved it in his monumental 1946 thesis, but the message has evidently not fully sunk in yet. The different Lie algebras underlying classical versus QM fare spectacularly differently under the Q2 map. People draw guidance/inspiration from it (Q2) when extending classical physics (e.g. the Boltzmann factor, or angular momentum) to the quantum domain, which is what "assume" means here: a background shadow; but they are very careful to avoid proving the earth is thereby flat, and delight in focussing on the novel, genuine, quantum behaviors involved.
Here is a stark example. Absorbing superfluous pesky constants in the variables, the classical oscillator hamiltonian is $H= \tfrac{1}{2} (p^2+ x^2)$. You have quantized it in introductory QM as
$$
\hat H= \tfrac{1}{2} (\hat p^2+ \hat x^2),
$$
but note neither of the summands commutes with the sum, and hence eigenvectors and eigenvalues are not shared.
Now, in QM, you have studied the Boltzmann operator,
$$
\exp (-\beta\hat H)= \exp (-\beta (\hat p^2+ \hat x^2)/2 ),
$$
and you might have inferred it as a slam-dunk application of Q2.
However, the classical ancestor of this is
$$
\exp (- \beta H )= \exp (- \beta( p^2+ x^2)/2 )\\
= \exp (- \beta p^2/2 )\exp (- \beta(x^2/2 )= ... ,
$$
or any algebraic rearrangement of the canonical variables.
You then appreciate Q2 will give you an infinity of differing, inequivalent answers, depending on which rearrangement of classical canonical variables you start with.
It turns out that in the maximally symmetric arrangement of $\hat x$ and $\hat p$ operators, dubbed "Weyl ordering", the classical variables expression ("Wigner image") yielding the above simple QM one is a famously magnificent mess,
$$
\exp_\star \left ( -\beta H \right )=
\left ( \cosh ( \hbar \beta / 2 )\right ) ^{-1}
\exp\left ( \frac{-2}{\hbar} H\tanh( \hbar \beta /2)\right ) ,
$$
as it is not even classical-looking: even though the canonical variables are classical, there is nontrivial $\hbar$ dependence due to the $\star$ operator which entails $\hbar$ and was invented by Groenewold to ensure this Q2-substitute is consistent.
So Q2 "assumed" is a shared metaphor: one tastefully chooses what to extend, by inspired guesswork, and develops, by experience, a sixth-sense of avoiding the problematic and the inconsistent. Trying to quantize problems in messy recondite geometry manifolds is still a challenge, problems to be solved. Q2 will never get you there by itself.
Now, to be sure, if only one observable (here H) is involved, there is no
non-commutativity structure to snag, and the sole observable is the collection of its eigenvalues, so, in a trivial way, Q2 works and is assumed. The mayhem starts when the observable is a function of others, (x,p), and ordering problems arise, as illustrated.
