|q⟩ Bad Qubits

beginner · Physics · Quantum Numbers & the Hydrogen Atom (Intro)

Orbital Angular Momentum ℓ

Classical mechanics gives us a continuous angular momentum vector L=r×p\mathbf{L} = \mathbf{r} \times \mathbf{p} that can point in any direction and take any magnitude. Quantum mechanics changes both of those facts: both the magnitude and the component along any chosen axis are quantized, and the quantization is governed by the orbital angular momentum quantum number \ell.

What ℓ quantizes

The magnitude of the orbital angular momentum is not free to vary continuously. It is restricted to the discrete values

L=(+1),=0,1,2,,n1,|\mathbf{L}| = \hbar\sqrt{\ell(\ell+1)}, \qquad \ell = 0, 1, 2, \ldots, n-1,

where nn is the principal quantum number and =h/(2π)\hbar = h/(2\pi) is the reduced Planck constant.

The constraint 0n10 \le \ell \le n-1 comes directly from solving the Schrödinger equation in spherical coordinates. Requiring the angular wave function to be single-valued and normalizable forces \ell to be a non-negative integer. The upper bound n1\ell \le n-1 then comes from the radial equation for the Coulomb potential: a normalizable radial solution exists only when n=nr++1n = n_r + \ell + 1 with the radial quantum number nr=0,1,2,n_r = 0, 1, 2, \ldots, so \ell can be at most n1n-1.

A few values to build intuition:

| \ell | Letter label | (+1)\sqrt{\ell(\ell+1)} | L|\mathbf{L}| | |--------|-------------|----------------------|----------------| | 0 | s | 0 | 0 | | 1 | p | 2\sqrt{2} | 2\hbar\sqrt{2} | | 2 | d | 6\sqrt{6} | 6\hbar\sqrt{6} | | 3 | f | 12\sqrt{12} | 12\hbar\sqrt{12} |

The letter labels (s, p, d, f, ...) come from spectroscopic notation and appear in electron shell configurations such as 1s22s22p61s^2\,2s^2\,2p^6.

Why ℓ = 0 is surprising

For =0\ell = 0 the magnitude is exactly zero — the electron has no orbital angular momentum at all. Classically this would mean the electron flies straight through the nucleus, which is clearly wrong. Quantum mechanically the s-states are spherically symmetric probability clouds with no preferred direction; there is no classical orbit, so "no angular momentum" makes sense.

The shape connection

The quantum number \ell also controls the shape of the orbital:

Each increase in \ell adds one more nodal surface and one more lobe structure to the angular part of the wave function.

Counting the m_ℓ states

Given \ell, the magnetic quantum number mm_\ell specifies the component of L\mathbf{L} along a chosen axis:

Lz=m,m{,+1,,1,}.L_z = m_\ell\,\hbar, \qquad m_\ell \in \{-\ell,\,-\ell+1,\,\ldots,\,\ell-1,\,\ell\}.

There are exactly 2+12\ell + 1 allowed values of mm_\ell. For example, a dd-orbital (=2\ell = 2) has 2(2)+1=52(2)+1 = 5 distinct mm_\ell values, giving the five dd-orbitals familiar from chemistry.

Try it

This is a numerical exercise — your code should return a number. For =3\ell = 3 (an ff-orbital), how many distinct values can mm_\ell take? Use the formula 2+12\ell + 1 derived above.

Run your code to see the quantum state.

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