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Various stackexchange (SE) posts have made it clear that the quantization of the energies in the Schrödinger equation arises due to the presence of boundary conditions. See for reference this, this and that question and their respective answers.

I am however confused about how Heisenberg's uncertainty principle which can be derived from the commutation relations of the respective operators: $$ [\hat{x}, \hat{p}] = \imath\hbar \quad\Rightarrow\quad \Delta x\Delta p \geq \frac{\hbar}{2}$$ can be used to explain quantization of energies as claimed in SE posts like this one or that one, where the latter focuses on a semiclassical picture.

Can someone provide a specific example (electron in a square well, hydrogen atom, harmonic oscillator, etc.) where a problem in quantum mechanics is solved using the Schrödinger equation, and the quantization of the resulting energies can clearly be linked to the Heisenberg uncertainty principle (or alternatively the canonical commutation relations) without invoking any boundary conditions?

xabdax
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I am however confused about how... $$ [\hat{x}, \hat{p}] = \imath\hbar \quad\Rightarrow\quad \Delta x\Delta p \geq \frac{\hbar}{2}.$$ can be used to explain quantization of energies as claimed in SE posts like.

A simple example where the differential equation's boundary conditions can be hidden under the rug of algebraic formalism is the quantum simple harmonic oscillator. (But at the end of the day, as we will see, you still need the boundary conditions!)

... where a problem in quantum mechanics is solved using the Schrödinger equation

For the simple harmonic oscillator, you solve the Schrodinger equation: $$ -\frac{1}{2}\frac{d^2 \psi}{dx^2} + \frac{1}{2}x^2\psi = E\psi\;, $$ subject to the boundary conditions that $\psi(x)\to 0$ as $x\to \pm \infty$. (For ease of writing I set $\hbar=m=k=1$.)

After solving the differential equation, you end up with quantized energy levels.

...and the quantization of the resulting energies can clearly be linked to the Heisenberg uncertainty principle (or alternatively the canonical commutation relations) without invoking any boundary conditions?

In the algebraic formalism we define $$ \hat a = \frac{1}{\sqrt{2}}(\hat x+i\hat p) $$ and $$ \hat a^\dagger = \frac{1}{\sqrt{2}}(\hat x-i\hat p) $$ and we use the relation $$ [\hat x,\hat p]=i $$ to see that $$ [\hat a,\hat a^\dagger]=1 $$ and so $$ \hat H=\hat a^\dagger \hat a + \frac{1}{2}\;. $$

And again we end up with quantized energies.

This follows since there is a lowest energy state such that $$ \hat a|0\rangle = 0\;\;, $$ which has energy $1/2$.

And we can create the other energy eigenstates by acting on $|0\rangle$ with $\hat a^\dagger$ like $$ |1\rangle = \hat a^\dagger|0\rangle $$ which has energy $3/2$. And so on in integer (i.e., quantized) steps.


But now you might rightfully wonder: Where did the boundary conditions go in the algebraic formalism?

The answer is that you still must include boundary conditions. But, in the algebraic formalism, they are included in the definitions of operators.

For example, the domain of the operator $\hat p$ in the SHO problem is defined as $$ \mathcal{D}(\hat p) = \left\{ \psi(x)\in L^2| \frac{d\psi}{dx}\in L^2 \text{ and }\lim_{x\to\pm\infty}\psi(x)\to 0 \right\}\;. $$

You must make such a definition because if you do not then $\hat p$ is not hermitian. To see this, consider $$ \langle \chi|\hat p|\psi\rangle =-i\int_{-\infty}^\infty dx \chi^*(x)\frac{d\psi}{dx} $$ $$ =\left[\int_{-\infty}^{\infty}(-i\frac{d\chi}{dx})^*\psi(x)\right] -i\left.\chi^*\psi\right|^{\infty}_{-\infty}\;, $$ where the last term is not zero unless you use the boundary conditions.

So, for example, if we do not include the proper boundary conditions in the operator definition for $\hat p$ then the thing we called $\hat a^\dagger$ is not really the hermitian conjugate of the thing we called $\hat a$, which is a problem.

hft
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There are two slightly different meanings of quantisation that is often left unstated, that you seem to be mixing up.

The statement that is common to both types of quantisation appears in the equation $$\tag1E=n\hslash\omega$$ in that there can be $n\in\mathbb Z^+_0$ "particles", each of energy $\hslash\omega$ in the system.

Here comes the important point: The quantisation of $\omega$ is due to boundary conditions whereas the quantisation of $n$ is due to commutation relations. Neither of them are related to Heisenberg's Uncertainty Principle (HUP) except indirectly via both $n$-quantisation and HUP's relationship to the commutation relations.


Consider completely free photons in completely empty universe. Then there are no boundary conditions and $\omega$ is not quantised at all. However, to explain Planck's blackbody radiation, you need to introduce the quantisation of the $n$ type that leads back to Equation (1), and it is clear from the simplest consideration of quantum electrodynamics (QED), a form of quantum field theory (QFT), that both the bosonic character of photons (spin-statistics theorem) and this particular form of quantisation come from the commutation relations of the field operators.

Of all the other cases whereby $\omega$ has a discrete spectrum (ignoring the continuous spectrum when they also exist, e.g. Hydrogen continuum states, because that part is already handled above), the reason for the discrete spectrum is due completely to boundary conditions. In particular, if you want the wavefunctions to be normalisable, as opposed to the continuum's normalisation conditions, then you will have the boundary conditions. For a slightly different perspective, Freericks et. al. recently revisited Schrödinger's original solution of the Hydrogen atom, which is somewhat akin to doing a Laplace transform on the Schrödinger's equation, and obtained the discreteness in another manner. In either case, this kind of quantisation has absolutely nothing whatsoever to do with HUP, because it has nothing to do with commutation relations.