Electron Spin and the Pauli Principle
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You should be comfortable with the four quantum numbers (\(n, l, m_l\)) and the concept of atomic orbitals as spatial probability distributions. Familiarity with the previous lecture on radial distribution is helpful but not strictly required.
Why this matters
Without electron spin and the Pauli exclusion principle, matter as we know it would not exist.
Classical physics predicts that electrons in atoms should spiral into the nucleus; and even in quantum mechanics, without one extra rule, all the electrons of an atom would crowd into the lowest orbital. This does not happen. The quantum mechanical description introduces an intrinsic angular momentum called spin, which provides a fourth quantum number. Combined with the Pauli exclusion principle, this spin property dictates how electrons populate orbitals, directly determining the structure of the periodic table, the nature of chemical bonding, and the magnetic properties of materials. Understanding this is the bridge between the isolated atom and the behaviour of bulk matter.
The Fourth Quantum Number
Imagine an electron not just as a particle orbiting a nucleus, but as a tiny spinning top. While the first three quantum numbers (\(n, l, m_l\)) describe the size, shape, and orientation of the orbital, they do not distinguish between two electrons that might occupy the exact same spatial region. Nature requires a way to differentiate them. This is where spin enters. Electron spin is an intrinsic property, not a literal mechanical rotation, but it behaves mathematically like angular momentum. It has two possible orientations relative to an arbitrary axis: "spin up" and "spin down." This binary nature is crucial because it means that even if two electrons are in the same orbital, they can be distinguished by their spin state. This distinction is the key that allows atoms to hold more than one electron without violating fundamental quantum laws.
Quantifying Spin
Spin is quantized, meaning it can only take specific discrete values. For an electron, the spin quantum number \(s\) is always \(\tfrac{1}{2}\). The projection of this spin onto a chosen axis (usually the z-axis) is described by the magnetic spin quantum number \(m_s\). Because \(s = \tfrac{1}{2}\), \(m_s\) can only take two values: \(+\tfrac{1}{2}\) or \(-\tfrac{1}{2}\). These are conventionally referred to as spin-up and spin-down.
The magnitude of the spin angular momentum \(S\) is given by the formula \(\sqrt{s(s+1)}\hbar\). Substituting \(s = \tfrac{1}{2}\), we find the magnitude is \(\sqrt{\tfrac{1}{2}(\tfrac{3}{2})}\hbar = \sqrt{\tfrac{3}{4}}\hbar = \tfrac{\sqrt{3}}{2}\hbar\). This value is fixed for all electrons, regardless of the atom or the orbital they occupy. Spin is an intrinsic property of the electron itself, not of its environment.
The Pauli Exclusion Principle
The Pauli exclusion principle is a fundamental law of quantum mechanics with profound consequences. It states that no two electrons in the same atom can have the identical set of all four quantum numbers (\(n, l, m_l, m_s\)). Since the first three numbers define the specific orbital, this implies that a single orbital can hold a maximum of two electrons, and those two electrons must have opposite spins.
If we attempt to place a third electron into the same orbital, it would have to share the same \(n, l, m_l\) as the first two. To be distinct, it would need a unique \(m_s\). However, only two values of \(m_s\) exist. Therefore, a third electron is forbidden from occupying that orbital. It must move to a higher energy orbital. This principle is the direct reason why the periodic table has its specific shape and why elements have distinct chemical properties based on their electron configurations.
Consequences for Orbital Capacity
The combination of the Pauli principle and the degeneracy of orbitals determines the maximum electron capacity of each subshell. A subshell is defined by a specific \(n\) and \(l\). The number of orbitals in a subshell is given by \(2l + 1\) (since \(m_l\) ranges from \(-l\) to \(+l\)). Since each orbital holds two electrons (one spin-up, one spin-down), the maximum capacity of a subshell is \(2(2l + 1)\).
- s subshell (\(l=0\)): 1 orbital \(\times\) 2 electrons = 2 electrons max.
- p subshell (\(l=1\)): 3 orbitals \(\times\) 2 electrons = 6 electrons max.
- d subshell (\(l=2\)): 5 orbitals \(\times\) 2 electrons = 10 electrons max.
- f subshell (\(l=3\)): 7 orbitals \(\times\) 2 electrons = 14 electrons max.
These capacities (2, 6, 10, 14) are why the rows of the periodic table hold 2, 8, 8, 18, 18, 32 and 32 elements. The Pauli principle effectively "fills up" the available states, forcing subsequent electrons into higher energy levels, which creates the shell structure we observe.
The result
The building-up principle
The ground-state electron configuration of an atom is obtained by filling the atomic orbitals of the previous result one electron at a time, subject to three rules: (1) the Madelung rule: orbitals fill in order of increasing \(n+l\), and for orbitals sharing the same \(n+l\), in order of increasing \(n\); (2) the Pauli exclusion principle: no orbital holds more than two electrons, and those two must have opposite spin (\(m_s=+\tfrac12\) and \(m_s=-\tfrac12\)); (3) Hund's rule: within a set of degenerate orbitals (equal \(n\) and \(l\), differing only in \(m_l\)), electrons occupy separate orbitals with parallel spin before any orbital is doubly occupied.
A common misconception is that electron spin is a literal physical rotation of the electron around its own axis. If an electron were a classical sphere of radius \(\sim 10^{-15}\ \mathrm{m}\) rotating with the angular momentum required for spin \(\tfrac{1}{2}\), its surface would need to move faster than the speed of light, violating special relativity. Spin is an intrinsic quantum property with no classical analogue; it is not motion in space, but a fundamental degree of freedom. C
Worked example
Problem. Determine the maximum number of electrons that can occupy the \(n=3\) shell of an atom, and list the possible sets of quantum numbers for the first two electrons in the \(3d\) subshell.
- Identify the allowed subshells for \(n=3\). The quantum number \(l\) can range from \(0\) to \(n-1\), so \(l = 0, 1, 2\). These correspond to \(3s\), \(3p\), and \(3d\) subshells.
- Calculate the capacity of each subshell using the formula \(2(2l+1)\):
- \(3s\) (\(l=0\)): \(2(2(0)+1) = 2\) electrons.
- \(3p\) (\(l=1\)): \(2(2(1)+1) = 6\) electrons.
- \(3d\) (\(l=2\)): \(2(2(2)+1) = 10\) electrons.
- Sum the capacities to find the total for the \(n=3\) shell: \(2 + 6 + 10 = 18\) electrons.
- For the \(3d\) subshell, the first electron occupies one of the five \(m_l\) orbitals (say, \(m_l = -2\)) with spin \(m_s = +\tfrac{1}{2}\). The second electron must have a different set of quantum numbers. According to Hund's rule (which we will discuss in the next lecture), it will occupy a different orbital with parallel spin, but the Pauli principle alone only requires that it not be identical to the first. If we simply list valid distinct states for the first two electrons in the subshell (ignoring energy ordering for a moment), one valid pair is:
- Electron 1: \(n=3, l=2, m_l=-2, m_s=+\tfrac{1}{2}\)
- Electron 2: \(n=3, l=2, m_l=-1, m_s=+\tfrac{1}{2}\)
Units check. The result is a dimensionless count of particles, which is consistent with the question asking for a number of electrons.
Three quick tests
- What are the two possible values of the magnetic spin quantum number \(m_s\) for an electron?
Answer
\(+\tfrac{1}{2}\) and \(-\tfrac{1}{2}\). - According to the Pauli exclusion principle, what is the maximum number of electrons that can occupy a single atomic orbital?
Answer
Two, provided they have opposite spins. - How many electrons can a \(p\) subshell hold in total?
Answer
Six electrons (three orbitals, each holding two).
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Every lecture and every result in this unit, with prerequisites and threads.
Lecture notes drafted with a local model and checked line by line by the editor; every number in the worked example was recomputed.