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Quiz ​

Question 1 — Valid or Invalid Quantum Numbers? ​

For each set of quantum numbers below, state whether it is valid or invalid, and explain why.

Recall the allowed ranges:

Quantum numberSymbolAllowed values
Principaln1,2,3,… (positive integers only)
Azimuthalℓ0,1,…,n−1
Magneticmℓ−ℓ,…,0,…,+ℓ
Spinms+12 or −12 only

Set A: n=1, ℓ=1

Answer

Invalid. ℓ must satisfy 0≤ℓ≤n−1. For n=1, the only allowed value is ℓ=0. Setting ℓ=1 violates this constraint — there is no p subshell in the first shell.


Set B: n=2, ℓ=1, mℓ=−1, ms=+32

Answer

Invalid. The spin quantum number ms can only take the values +12 or −12. The value +32 is not allowed — it would correspond to a higher spin than an electron possesses. The other three numbers (n=2, ℓ=1, mℓ=−1) are all valid on their own.


Set C: n=3, ℓ=1, mℓ=2

Answer

Invalid. mℓ must satisfy −ℓ≤mℓ≤+ℓ. For ℓ=1, the allowed values are mℓ∈{−1, 0, +1}. The value mℓ=2 lies outside this range.


Set D: n=0

Answer

Invalid. n must be a positive integer: n≥1. Zero is not a valid principal quantum number — there is no zeroth shell.


Question 2 — Ground-State Configuration of Calcium ​

What is the ground-state electron configuration of Calcium (Ca, Z=20)?

Answer1s2 2s2 2p6 3s2 3p6 4s2

Why 4s before 3d? The Madelung (diagonal) rule fills subshells in order of increasing n+ℓ:

  • 4s: n+ℓ=4+0=4
  • 3d: n+ℓ=3+2=5

Since 4<5, the 4s subshell is lower in energy for light atoms and fills first. After 3p6 (at Z=18, argon), the next two electrons go into 4s, completing the configuration above.

The shorthand notation using the previous noble gas is:

[Ar] 4s2

Calcium is the last element before the 3d transition metals begin filling. At Z=21 (Scandium), the first 3d electron appears.


Question 3 — Meaning of the Wave Function ​

The wave function Ψ is complex-valued, yet every measurement of a quantum system returns a real number. What does Ψ represent, and how is a real, observable prediction extracted from it?

Answer

The wave function is not itself an observable quantity — it is a probability amplitude. The observable is its absolute square,

|Ψ(r,t)|2=Ψ∗Ψ,

which is real and non-negative. |Ψ(r,t)|2dV gives the probability of finding the particle in the small volume dV around r at time t.

Because the particle must be found somewhere, Ψ is normalized so that the total probability is 1:

∫|Ψ|2dV=1.

The complex phase of Ψ never shows up in a single measurement, but it is essential: it governs how quantum states interfere, which is what makes quantum mechanics differ from a classical probability theory.


Question 4 — Particle in a Box: Energies ​

A particle is confined to a one-dimensional box of length L.

(a) What is the ratio E3/E1 of the third energy level to the ground state? (b) Why can the particle never have exactly zero energy?

Answer

(a) The allowed energies are

En=n2π2ℏ22mL2,

so En∝n2. Therefore

E3E1=3212=9.

(b) The lowest allowed state is n=1, not n=0. Setting n=0 gives ψ(x)=Asin⁡(0)=0 everywhere — a particle that exists nowhere. The smallest genuine standing wave fits half a wavelength across the box and still carries

E1=π2ℏ22mL2>0.

This irreducible zero-point energy is a direct consequence of confinement: a perfectly localized, perfectly motionless particle is forbidden by the uncertainty principle.


Question 5 — Why Spherical Coordinates? ​

Why is the Schrödinger equation for the hydrogen atom solved in spherical coordinates rather than Cartesian, and what two equations does separation of variables produce?

Answer

The Coulomb potential depends only on the distance from the nucleus:

V(r)=−e24πϵ0r.

In Cartesian coordinates that distance is r=x2+y2+z2, which tangles all three variables together. Spherical coordinates match the natural spherical symmetry of the atom, so the potential involves r alone.

Writing the wave function as a product Ψ(r,θ,ϕ)=R(r)Y(θ,ϕ) and separating splits one hard 3-D problem into two simpler ones:

  • the radial equation (in r) — determines the energy levels and the principal quantum number n;
  • the angular equation (in θ,ϕ) — determines the orbital shapes and the quantum numbers ℓ and mℓ.

The two equations are linked by the separation constant ℓ(ℓ+1).


Question 6 — Orbitals in a Subshell ​

For the d subshell:

(a) What are the allowed values of mℓ? (b) How many orbitals does the subshell contain? (c) How many electrons can it hold in total?

Answer

A d subshell has ℓ=2.

(a) mℓ takes every integer from −ℓ to +ℓ:

mℓ∈{−2, −1, 0, +1, +2}.

(b) Each value of mℓ labels one orbital, so there are 2ℓ+1=5 orbitals.

(c) By the Pauli exclusion principle each orbital holds 2 electrons (opposite spins), giving

2(2ℓ+1)=10 electrons

— exactly the width of the d-block.


Question 7 — Nodes of a 3p Orbital ​

How many radial nodes and how many angular nodes does a 3p orbital have? What is the total number of nodes?

Answer

A 3p orbital has n=3 and ℓ=1.

  • Angular nodes =ℓ=1 — one nodal plane through the nucleus, which is what splits a p orbital into two lobes.
  • Radial nodes =n−ℓ−1=3−1−1=1 — one spherical shell of zero probability.
  • Total nodes =n−1=2.

The rule total nodes =n−1 holds for every orbital. The value of ℓ decides how many of those nodes are angular; the remainder, n−ℓ−1, are radial.


Question 8 — Hydrogen Energy and Subshell Splitting ​

(a) Using En=−13.6 eV/n2, find the energy of the n=2 level of hydrogen. (b) In hydrogen the 2s and 2p subshells have the same energy, but in a multi-electron atom 2s lies below 2p. Why?

Answer

(a)

E2=−13.6 eV22=−13.6 eV4=−3.40 eV.

(b) In hydrogen — a single electron — the energy depends only on n, so 2s and 2p are degenerate. In a multi-electron atom this degeneracy is broken by penetration and shielding. The 2s radial distribution has a small inner peak that lets the electron penetrate the 1s core and feel a larger effective nuclear charge Zeff. The 2p orbital has a node at r=0 and is held further out, so it is shielded more effectively. Penetrating deeper, the 2s electron is more tightly bound — lower in energy — hence E2s<E2p.


Question 9 — Hund's Rule and Nitrogen ​

State the Pauli exclusion principle and Hund's rule. Then apply them to nitrogen (Z=7): give its ground-state 2p occupation, the number of unpaired electrons, and whether it is paramagnetic or diamagnetic.

Answer
  • Pauli exclusion principle: no two electrons in an atom may share all four quantum numbers (n,ℓ,mℓ,ms). Hence an orbital holds at most 2 electrons, with opposite spins.
  • Hund's rule: within a subshell, electrons occupy separate orbitals with parallel spins before any orbital is doubly filled — this minimizes electron–electron repulsion.

Nitrogen's configuration is 1s2 2s2 2p3. The three 2p electrons each take a different 2p orbital with parallel spins:

2p:↑  ↑  ↑

That leaves 3 unpaired electrons, so nitrogen is paramagnetic. With its half-filled 2p subshell, it is in fact the most paramagnetic atom of period 2.


Question 10 — Why Periods 6 and 7 Hold 32 Elements ​

Periods 6 and 7 of the periodic table each contain 32 elements. Derive this number from the quantum-mechanical subshell capacities.

Answer

A period corresponds to filling one complete set of subshells in Aufbau order. Each subshell holds 2(2ℓ+1) electrons:

s=2,p=6,d=10,f=14.

Periods 6 and 7 are the first to draw on all four block types — they fill an s, an f, a d and a p subshell:

2+14+10+6=32.

For period 6 the sequence is 6s→4f→5d→6p; for period 7 it is 7s→5f→6d→7p. The 14 contributed by the f subshell is exactly the length of the lanthanide and actinide rows.

(Periods 4–5 omit the f block and hold 2+10+6=18; periods 2–3 omit both f and d and hold 2+6=8.)