2.3.13 · D1Modern Physics

Foundations — Quantum numbers n, l, mₗ, mₛ

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Before you can read the parent note, you must own every piece of its vocabulary. This page builds each symbol from the ground up: what it means in plain words, what picture it stands for, and why the topic cannot do without it. Read top to bottom — each item leans on the one before, and no quantum number is used before it is derived.


1. Angle, radius, and the three coordinates

Before any physics, we need a way to say where a point is around a nucleus.

The everyday way is : walk east, walk north, walk up. But an atom is round — the pulling force from the nucleus is the same in every direction at a given distance. So we use coordinates that match that roundness: spherical coordinates.

Figure — Quantum numbers n, l, mₗ, mₛ

Look at the figure: is the length of the amber arrow, is how far that arrow leans away from straight-up, and is how far around the equator you have swept starting from the -axis. Every point in space is named by exactly one triple .

Why the topic needs this: the electron wave is written as (we meet in §3). Later, each of the three "shape counts" will come from one of these three directions — one from , one from , one from .


2. What and radians mean

ran from to , not to . Why?


3. The wave (psi)

Why the topic needs it: the whole idea "the electron is a standing wave" is the statement that the electron is described by . Quantum numbers are labels on the allowed shapes.


4. Standing waves and "fitting a whole number of bumps"

This is the heart of where integers come from.

Figure — Quantum numbers n, l, mₗ, mₛ

Look at the figure: on the string you can fit 1 bump, 2 bumps, 3 bumps — but never bumps, because the loose end wouldn't line up. The number of bumps is forced to be a whole number. That whole number is the ancestor of every quantum number.


5. Complex numbers and — and the birth of

The -wave is written . That and that scare people. Here is all you need.

Figure — Quantum numbers n, l, mₗ, mₛ

Now we derive our first quantum number. Bend the electron's -direction into a ring (the circle of §1, starting at ). Walking one full loop takes you from to , and the wave must return to the same value — otherwise it has a rip:

What this says: going around the circle times must land you exactly back at the start. That is only true when is a whole number.

Why the topic needs it: is the first integer that "falls out" of a match-yourself condition. Its sign is a real physical thing — it says which way the electron fog is circulating.


6. The -wave and the birth of

The -direction gave . Now the tilt direction gives a second whole number.

The tilt-wave must obey the polar piece of Schrödinger's equation (called Legendre's equation). You do not need to solve it — you need one fact about it.

When you enforce "finite at both poles," the maths (Legendre's equation) only allows solutions when a certain constant equals with a whole number — and only when . Any other value makes the tilt-wave shoot off to infinity at a pole, which is unphysical (a fog can't be infinitely thick at one point).

Figure — Quantum numbers n, l, mₗ, mₛ

Why makes sense: you cannot wrap around the equator more sharply than the overall pattern is wrinkled. A very "calm" pattern (small ) simply has no room for a fast horizontal wrap (large ). Look at the figure: as grows, more slots open up on both the negative and positive sides.


7. The -wave and the birth of

Two down, one to go. The radial direction gives the last of the wave-equation trio.

When you enforce "the wave dies out as ," the radial equation only has well-behaved solutions for whole-number values , and only when . This same condition also freezes the allowed energies (that is where the parent note's comes from).

Why the topic needs it: is the master label — it sets energy and size, and it caps how wrinkled () the fog may be. See Hydrogen Atom Energy Levels for the energies it produces.


8. Vectors, the arrow , and the constant

We now have . To connect and to real physics we need one more picture: the arrow of angular momentum.

Figure — Quantum numbers n, l, mₗ, mₛ

Now the two integers earn their physical jobs:

  • sets the arrow's length: .
  • sets the arrow's shadow: .

Look at the figure: the cyan arrow is , and its shadow on the vertical -axis is . A shadow is always shorter than the arrow unless the arrow points straight up — this is exactly why the parent note insists (space quantization). And because can be negative, the shadow can point down () as well as up.

Why the topic needs it: an state has — a perfectly round, non-swirling fog. See Angular Momentum in Quantum Mechanics for the full arrow story.


9. Spin: the numbers and

The three numbers all came from the wave equation. There is a fourth label that does not come from that equation — it was forced on us by experiment.

Just as the tilt-arrow had a shadow with running in whole steps from to , the spin-arrow has a shadow whose label runs in whole steps from to .

Figure — Quantum numbers n, l, mₗ, mₛ

Why exactly two values? Because , the ladder from to has only the two rungs . This is precisely what the Stern-Gerlach Experiment showed: a beam of atoms split into exactly two spots — the direct fingerprint of a two-valued built-in magnet.


10. The Schrödinger equation (the machine that makes all this)

You don't have to solve it (that's Schrödinger Equation's job). You only need: it is the sieve; the first three quantum numbers are the labels on whatever passes through.


Prerequisite map

Spherical coordinates r theta phi

Wavefunction psi

Radians and pi

Standing waves

Complex numbers and e^i phi

phi ring wave gives m_l

theta pole wave gives l

r fade-out wave gives n

Schrodinger equation

Vectors and shadow L_z

Angular momentum L

Reduced constant h-bar

Spin from Stern-Gerlach

s and m_s

Full set n l m_l m_s


Equipment checklist

Cover the right side and test yourself. If you can answer all of these, the parent note 2.3.13 will read smoothly.

What are the three spherical coordinates and what does each measure?
= distance from nucleus, = tilt down from the -axis, = angle swept anticlockwise around the horizontal circle starting from .
How many radians is one full turn around a circle?
radians (equal to ).
What does mean, and what do you actually measure?
is a number the electron carries at each point; the measurable thing is , the probability of finding the electron there.
Why can a standing wave hold only a whole number of bumps?
The wave must match its boundary conditions (join up smoothly), so only wavelengths that fit exactly survive — fractional bumps leave a mismatch.
What does trace out as increases?
A point walking anticlockwise around the unit circle; .
Which boundary condition gives , and what does it force?
The -ring must match after one loop, so forces to be an integer (positive, zero, or negative).
What do positive, zero, and negative mean physically?
Positive = wave wraps anticlockwise, negative = wraps clockwise, zero = no wrap; the range is .
Which boundary condition gives , and what range does it allow?
The -wave must stay finite at both poles; this forces and caps so .
Which boundary condition gives , and what does it cap?
The radial wave must fade out as ; this forces and caps .
For a vector , what is geometrically, and why is it ?
is the arrow's shadow (projection) on the -axis; a shadow is never longer than the arrow itself.
What is and what role does it play?
The smallest chunk of angular momentum ( J·s); angular momentum comes in whole multiples of it.
What are and , and why does take exactly two values?
is the fixed spin size; runs from to in whole steps, giving only and .
Which experiment forced the fourth quantum number on us?
The Stern-Gerlach Experiment, where a beam split into exactly two.