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Quantum Mechanical Model: Quantum Numbers, Orbitals and Configuration

Moving electrons also behave like waves: λ = h/mv (de Broglie). Because of this we cannot know exact position and momentum together: Δx·Δp ≥ h/4π (Heisenberg). So we drop sharp orbits and use orbitals: regions where the electron is likely to be, from the Schrödinger equation (ψ² gives probability). Four quantum numbers describe each electron: n (shell, size, energy), l (subshell, shape: 0 to n−1), mₗ (orientation: −l to +l) and mₛ (spin: +½ or −½). s is spherical, p is dumbbell, d is mostly four-lobed. Electrons fill by the Aufbau (n + l) rule, Pauli principle (max 2, opposite spins) and Hund's rule (single first). Half-filled and fully filled subshells are extra stable, so Cr is 3d⁵4s¹ and Cu is 3d¹⁰4s¹.

🎬 Step-by-step story

  1. An electron is a tiny particle but also a wave, with λ = h/mv. Round an orbit only a whole number of waves fits; a broken wave cancels itself.
  2. Try to pin down where the electron is (make the cloud small): its momentum arrows spread wide. You can never know both exactly: Δx·Δp ≥ h/4π.
  3. So we draw an orbital: a cloud of dots, thick where the electron is likely to be. 1s is a fuzzy ball; 2s is bigger with an empty shell (node) inside.
  4. Every orbital has an address: n (shell), l (shape), mₗ (direction). Each electron also has spin mₛ = +½ or −½. Change n and l to see new orbitals.
  5. Shapes: s is a ball, p is a dumbbell along x, y or z, d mostly has four lobes (dz² is a dumbbell with a ring). mₗ turns the orbital.
  6. Free play: choose Z from 1 to 30 and watch electrons fill the boxes: lowest energy first, two opposite spins per box, singles before pairs. Try Cr (24) and Cu (29).

Tip: drag the 3D scene to turn it. Use two fingers to zoom.

🤔 Common doubts, cleared

If an electron is a wave, why don't we see a cricket ball as a wave?

λ = h/mv. A ball's mass is huge compared to an electron, so its λ is around 10⁻³⁴ m, far too small to show any effect.

Can't a better instrument beat the uncertainty principle?

No. It is a property of nature, not of instruments. Any light able to locate the electron sharply also kicks it hard.

What exactly is the difference between orbit and orbital?

An orbit is a fixed circle with exact position at every moment. An orbital is a 3D cloud showing where the electron is likely to be; it has no fixed path.

Why can't l be equal to n?

The solutions of the equation only allow l from 0 to n − 1. That is why shell 1 has only s, shell 2 has s and p.

Why do the p orbitals have zero chance at the nucleus?

A p orbital has a nodal plane through the nucleus: the two lobes have opposite signs of ψ, and ψ² is zero on the plane between them.

Why does 4s fill before 3d?

By the (n + l) rule 4s has 4 and 3d has 5. The 4s electron penetrates closer to the nucleus and is less shielded. Watch Z = 19, 20 then 21 in free play.

Why are Cr and Cu exceptions?

Half-filled (d⁵) and full (d¹⁰) subshells are extra stable due to symmetry and exchange energy. Set Z = 24 and 29 and watch the 4s electron move.

Dual behaviour of matter: de Broglie

Light behaves as a wave and as a particle. In 1924 de Broglie said matter should too: any moving particle has a wavelength

λ = h/mv = h/p (p = momentum).

For a cricket ball λ is so tiny (about 10−34 m) that no wave effect can be seen. For an electron, with its very small mass, λ is about the size of an atom, so wave effects matter. Electron diffraction proved it, and the electron microscope uses it.

Link to Bohr: if a whole number of electron waves fits on an orbit, 2πr = nλ = nh/mv, which gives mvr = nh/2π: exactly Bohr's rule.

Heisenberg's uncertainty principle

It is impossible to know the exact position and the exact momentum (or velocity) of an electron at the same time:

Δx × Δp ≥ h/4π, or Δx × Δv ≥ h/(4πm).

Why: to "see" an electron you must hit it with light of wavelength smaller than the region you want to measure. Such light has high energy and knocks the electron, changing its momentum. The sharper the position, the fuzzier the momentum.

What it means: the idea of a fixed path (orbit) for an electron is meaningless, so Bohr's model must go. For big objects (a ball) the uncertainty is far too tiny to notice.

Quantum mechanical model and orbitals

Schrödinger (1926) wrote an equation for the electron as a wave. Its solutions are wave functions ψ. ψ itself has no simple meaning, but ψ² gives the probability density: how likely the electron is to be found at a point.

Quantum numbers

Quantum numberValuesTells us
Principal n1, 2, 3 … (K, L, M …)Shell, size and energy. Orbitals in shell n = n²; electrons = 2n².
Azimuthal l0 to n − 1 (s, p, d, f)Subshell and shape. Orbitals in a subshell = 2l + 1.
Magnetic mₗ−l … 0 … +lOrientation of the orbital in space.
Spin mₛ+½ or −½Spin direction of the electron (↑ or ↓).

Example: for n = 3, l can be 0, 1, 2 (3s, 3p, 3d); number of orbitals = 1 + 3 + 5 = 9 = 3²; electrons = 18.

Orbital angular momentum = √(l(l+1)) · h/2π.

Shapes of s, p and d orbitals

Energy of orbitals and the (n + l) rule

In hydrogen, energy depends only on n: 2s = 2p. In atoms with many electrons, energy also depends on l, because inner electrons shield outer ones, and s electrons get closer to the nucleus (penetrate) more than p, then d.

(n + l) rule: lower n + l means lower energy. If equal, lower n comes first. So 4s (4+0 = 4) fills before 3d (3+2 = 5).

Order: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s …

Filling rules: Aufbau, Pauli and Hund

  1. Aufbau principle: electrons go into the lowest-energy orbital first ("aufbau" = building up).
  2. Pauli exclusion principle: no two electrons in an atom can have all four quantum numbers the same. So one orbital holds at most two electrons, with opposite spins (↑↓).
  3. Hund's rule of maximum multiplicity: in orbitals of equal energy (p, d, f), electrons first go in singly, with parallel spins; pairing starts only after each orbital has one. So N (2p³) is ↑ ↑ ↑, not ↑↓ ↑.

Electronic configuration and stability

Write subshells with electron counts as superscripts: O (8) = 1s² 2s² 2p⁴; K (19) = 1s² 2s² 2p⁶ 3s² 3p⁶ 4s¹ = [Ar] 4s¹. The outermost electrons are valence electrons; the rest are core electrons.

Special stability of half-filled and fully filled subshells:

So Cr (24) = [Ar] 3d⁵ 4s¹, not 3d⁴4s², and Cu (29) = [Ar] 3d¹⁰ 4s¹, not 3d⁹4s².

Ions: remove electrons from the highest n first. Fe (26) = [Ar]3d⁶4s²; Fe²⁺ = [Ar]3d⁶; Fe³⁺ = [Ar]3d⁵ (half-filled, which is why Fe³⁺ is more stable).

Try it: fill and check

In the last story step, predict the configuration of nitrogen (Z = 7) and write it in your notebook with boxes and arrows. Then set Z = 7 and check that the three 2p electrons are single and parallel. Then compare Z = 23, 24, 25: watch the 4s electron move into 3d at Cr.

Board exam corner

Common questions: de Broglie wavelength and uncertainty numericals (2–3 marks); possible/impossible quantum number sets; number of orbitals/electrons in a shell; nodes; shapes of orbitals (diagram); state and explain Aufbau, Pauli, Hund; configurations of Z = 1–30 with Cr and Cu exceptions and why.

Key formulas and definitions

Worked examples

1. Find the de Broglie wavelength of a 0.1 kg ball moving at 10 m/s.

λ = h/mv = 6.626 × 10⁻³⁴ ÷ (0.1 × 10) = 6.626 × 10⁻³⁴ m. Far too small to notice.

2. Find the de Broglie wavelength of an electron (m = 9.1 × 10⁻³¹ kg) moving at 2.19 × 10⁶ m/s.

λ = 6.626 × 10⁻³⁴ ÷ (9.1 × 10⁻³¹ × 2.19 × 10⁶) = 6.626 × 10⁻³⁴ ÷ 1.993 × 10⁻²⁴ = 3.32 × 10⁻¹⁰ m = 332 pm, about the size of an atom. (This is 2πr for H's first orbit: one whole wave fits.)

3. A 25 g ball's position is known within 10⁻⁵ m. Find the minimum uncertainty in its velocity.

Δv = h/(4πmΔx) = 6.626 × 10⁻³⁴ ÷ (4 × 3.14 × 0.025 × 10⁻⁵) = 6.626 × 10⁻³⁴ ÷ 3.14 × 10⁻⁶ = 2.1 × 10⁻²⁸ m/s. Negligible.

4. An electron's position is known within 0.1 Å (10⁻¹¹ m). Find the minimum uncertainty in its velocity.

Δv = 6.626 × 10⁻³⁴ ÷ (4 × 3.14 × 9.1 × 10⁻³¹ × 10⁻¹¹) = 6.626 × 10⁻³⁴ ÷ 1.143 × 10⁻⁴⁰ = 5.8 × 10⁶ m/s. Bigger than its own speed in an atom, so a sharp orbit makes no sense.

5. Write the quantum numbers of all orbitals in the 3d subshell and the number of radial and angular nodes.

n = 3, l = 2, mₗ = −2, −1, 0, +1, +2 (five orbitals). Radial nodes = 3 − 2 − 1 = 0; angular nodes = 2.

6. Which sets are not possible? (a) n = 2, l = 2, mₗ = 0 (b) n = 3, l = 1, mₗ = −1 (c) n = 1, l = 0, mₗ = +1 (d) n = 4, l = 3, mₗ = −3

(a) impossible: l must be ≤ n − 1 = 1. (c) impossible: for l = 0, mₗ can only be 0. (b) 3p and (d) 4f are fine.

7. How many electrons in an atom can have n = 3 and mₛ = −½?

Shell n = 3 has n² = 9 orbitals. Each has one electron with mₛ = −½. Answer 9.

8. Arrange 4s, 3d, 4p, 5s by energy using the (n + l) rule.

4s: 4, 3d: 5, 4p: 5, 5s: 5. So 4s is lowest. Among n + l = 5, lower n first: 3d < 4p < 5s. Order: 4s < 3d < 4p < 5s.

9. Write configurations of Cr (24) and Cu (29) and explain.

Cr: 1s² 2s² 2p⁶ 3s² 3p⁶ 3d⁵ 4s¹. Cu: 1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s¹. Moving one 4s electron makes 3d half-filled (Cr) or full (Cu). These are more symmetric and have more exchange energy, so they are more stable.

10. How many unpaired electrons are in Fe³⁺ (Fe, Z = 26)?

Fe = [Ar] 3d⁶ 4s². Remove 4s² then one 3d: Fe³⁺ = [Ar] 3d⁵. By Hund's rule all five are single: 5 unpaired electrons.

Common mistakes

Practice quiz

1. de Broglie wavelength is given by:
2. For n = 3, the possible values of l are:
3. The shape of a p orbital is:
4. Which rule says an orbital can hold only two electrons with opposite spins?
5. The configuration of Cu (Z = 29) is:

Practice: answer these yourself

Type or choose your answer, then press Check. Use a hint if you are stuck; the full solution appears after you answer.

Frequently asked questions

What are the four quantum numbers?

Principal n (shell and energy), azimuthal l (subshell shape), magnetic mₗ (orientation) and spin mₛ (+½ or −½). Together they give each electron a unique address.

What is Heisenberg's uncertainty principle?

It is impossible to know the exact position and exact momentum of a tiny particle like an electron at the same time: Δx·Δp ≥ h/4π.

What are Aufbau principle, Pauli exclusion principle and Hund's rule?

Aufbau: fill lowest energy orbitals first. Pauli: no two electrons have all four quantum numbers the same, so max 2 per orbital with opposite spins. Hund: in equal-energy orbitals, put one electron in each before pairing.

Where this is taught

Canada (Ontario)Grade 12C. Structure and Properties Of Matter
ItalySecondaria di secondo grado – classe 3ªChemistry
ItalySecondaria di secondo grado – classe 4ªChemistry
Ukraine8 класStructure of the atom
Ukraine11 класReview and deepening of theory
CBSE (India)Class 11Structure of Atom
USA (Common Core, NGSS, AP)Grade 11Atomic Structure and Properties
South Korea고등학교 3학년The atomic world
Germany (Bavaria)Jahrgangsstufe 12Atomic structure and coordinate bonding
Germany (Bavaria)Jahrgangsstufe 13A quantum model of the atom
Russia11 классTheoretical foundations of chemistry
Russia11 классTheoretical foundations of chemistry
China高二Selective 2 Ch.1 Atomic structure and properties

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