QCC Notes
CLASS 11 · CHEMISTRYJEE MAIN × NEETहिंदी
§ 2.6NCERT Class 11 · Chemistry · Chapter 2

Quantum Mechanical Model of Atom: Quantum Numbers & Orbitals

Schrödinger’s equation replaced Bohr’s orbits with probability clouds — and out of its solutions fell four quantum numbers that give every electron a complete address. Shapes, nodes, capacities, the Aufbau energy ladder, and a live validator that polices every quantum-number set you dare to try.

01

What is the Quantum Mechanical Model? — Complete Theory

Bohr’s model — brilliant for hydrogen (§ 2.4) — collapsed under two blows from § 2.5: de Broglie showed the electron is a wave, and Heisenberg forbade knowing its exact path. If you cannot know the path, you cannot draw one. In 1926 Erwin Schrödinger wrote the equation that a wave-electron must obey — Hψ = Eψ — and solving it for the hydrogen atom changed the questions chemistry asks. Not “where is the electron?” but “how likely is the electron here?”

The solution ψ (psi) is the wave function — and it has no direct physical meaning by itself. Its square, |ψ|², is the probability density: large where the electron is likely to be found, small where it is not. Plot the region holding ~90–95% of that probability and you have an orbital — a fuzzy three-dimensional cloud, not a racetrack. Where Bohr had one number (n), the quantum atom needs four quantum numbers to pinpoint one electron — three falling out of the Schrödinger equation, one added by experiment:

Table 1 — The four quantum numbers: the electron’s full address
Quantum numberSymbolAllowed valuesWhat it fixesSource
Principaln1, 2, 3, …Shell — size and main energySchrödinger
Azimuthal (angular momentum)l0 to (n − 1)Subshell — shape: s, p, d, fSchrödinger
Magneticm−l … 0 … +lOrientation — 2l + 1 orbitalsSchrödinger
Spins+½, −½Electron’s intrinsic spinExperiment (Uhlenbeck–Goudsmit)

Read the l-row carefully — it carries the naming system. l = 0, 1, 2, 3 are written s, p, d, f (from sharp, principal, diffuse, fundamental — old spectroscopy jargon), and an orbital is named n + letter: 1s, 2s, 2p, 3d, 4f. Two legality rules follow instantly: l must satisfy l ≤ n − 1 (so 1p, 2d, 3f do not exist), and m must satisfy |m| ≤ l (a p subshell’s orientations run m = −1, 0, +1 — nothing outside).

Table 2 — Subshell census: orbitals, electrons, nodes
Subshelllm valuesOrbitals (2l+1)Electrons 2(2l+1)Angular nodes (= l)
s01 (0)120 — spherical
p13 (−1, 0, +1)361 — dumbbell
d255102 — cloverleaf
f377143 — complex

Roll this up to whole shells: shell n contains n² orbitals (n = 3 → one 3s + three 3p + five 3d = 9) and holds 2n² electrons (18). And every orbital carries internal architecture — nodes, surfaces of zero probability: radial (spherical) nodes = n − l − 1, angular (planar) nodes = l, and their sum is always n − 1. The split shifts between subshells of the same shell; the total never budges — a bookkeeping identity the exam loves to test.

Now the energy question — and here the quantum model draws a line between two universes. Hydrogen (one electron): energy depends only on n. All nine orbitals of n = 3 — 3s, 3p, 3d — are degenerate (equal energy), exactly as in Bohr’s Eₙ = −13.6/n² eV. Multi-electron atoms: energy depends on n + l. Electrons shield each other, so within a shell, lower l sinks lower: 3s < 3p < 3d. This single difference powers the Aufbau principle — fill orbitals in rising n + l order (ties broken by lower n): 1s → 2s → 2p → 3s → 3p → 4s → 3d → …, the sequence behind every electronic configuration you will ever write.

Two filling laws complete the machinery. Pauli’s exclusion principle: no two electrons in an atom share all four quantum numbers — an orbital (fixed n, l, m) can hold at most two electrons, and they must carry opposite spins. Hund’s rule: in degenerate orbitals, electrons first occupy separate orbitals singly with parallel spins before pairing — which is why nitrogen’s 2p³ is three half-filled orbitals, not one full and one empty. (The spin quantum number itself, remember, is the one the Schrödinger equation never produced — it entered through spectroscopy and keeps half-filled and fully-filled subshells extra stable.)

Probability density vs radial probability. ψ² is the probability density — the probability of finding the electron per unit volume at a point. For a 1s electron, ψ² is largest at the nucleus itself. But the chance of finding the electron at a distance r from the nucleus depends on the whole thin spherical shell at that distance, whose volume grows as 4πr²dr. The radial probability is therefore P(r) = 4πr²ψ²dr. For 1s it is zero at the nucleus, rises to a maximum at r = 0.529 Å — Bohr’s first radius, now the most probable distance rather than a fixed orbit — and then falls away. Each radial node appears as a zero in the curve: 2s (one radial node) shows two peaks, 3s (two nodes) shows three. In general the radial probability curve has (n − l) peaks, and the outermost peak is the tallest.

Exceptional configurations: chromium and copper. The Aufbau order predicts Cr (Z = 24) as [Ar] 3d⁴ 4s² and Cu (Z = 29) as [Ar] 3d⁹ 4s². The observed configurations are Cr: [Ar] 3d⁵ 4s¹ and Cu: [Ar] 3d¹⁰ 4s¹ — one 4s electron moves into 3d so that the d subshell becomes exactly half-filled (d⁵) or completely filled (d¹⁰). The 3d and 4s energies are close, so this small shift is repaid by extra stability, which has two sources.

(1) Symmetry. Half-filled and completely filled subshells have a symmetrical distribution of electrons. Electrons in the same subshell shield one another relatively poorly, so they are held more strongly by the nucleus. (2) Exchange energy. Electrons with parallel spins in degenerate orbitals can exchange positions, and each possible exchange releases energy (exchange energy) that stabilises the arrangement. The number of exchanges is greatest when the subshell is half-filled or completely filled: d⁵ with five parallel spins allows 10 exchanges (5 × 4 / 2), against only 6 for d⁴. This is also the reason behind Hund’s rule.

02

Visualising Orbitals & Validating Quantum Numbers

Chaar shapes, chaar numbers — the gallery shows what orbitals look like in cross-section, and the validator below polices your n-l-m-s sets like NTA does.

Orbital shapes and their nodes — 1s, 2s, 2p, 3d in cross-section FIG. 1 — ORBITAL SHAPES & NODES (CROSS-SECTIONS) 1s — spherical, no nodes 1s0 nodes spherical — l = 0 2s — spherical with one radial node 2s1 radial node dashed sphere = zero probability 2p — two lobes with one angular nodal plane 2p1 angular node dashed plane = nodal plane 3d — four lobes with two angular nodal planes 3d2 angular nodes four lobes along dashed planes radial (spherical) nodes = n − l − 1 · angular (planar) nodes = l · total = n − 1 2s → 1 + 0 = 1 · 3s → 2 + 0 = 2 · 3p → 1 + 1 = 2 · 3d → 0 + 2 = 2 · 4f → 0 + 3 = 3 same shell, same total — only the split between radial and angular shifts f orbitals (l = 3): seven orbitals, 3 angular nodes — shapes too intricate for a sketch p has 3 orientations (px, py, pz) · d has 5 · m labels which one
FIG. 1 — Cross-sections, not photographs: the 1s cloud is a solid sphere (no nodes), 2s hides a spherical zero-probability shell (1 radial node), 2p splits into two lobes across a nodal plane (1 angular node), and 3d spreads four lobes between two nodal planes. Count check: every orbital totals n − 1 nodes.
Try it live

Quantum Number Validator

Chaar numbers chuno — legal set par poora orbital profile milega; illegal par exact rule break pakda jayega. Try 2d ya m = 3 with l = 1 — validator nahi bachega.

Shape preview for the selected l value d — cloverleaf

Designation3d
Orbitals (2l+1)5
Electrons (2(2l+1))10
Shell n² / 2n²9 / 18
Radial nodes0
Angular nodes2
Total nodes2
Ang. momentum √(l(l+1))·h/2π2.449 h/2π

Legality rules enforced: l ≤ n − 1 and |m| ≤ l. Designations like 2d, 3f, 1p get caught instantly; m outside ±l gets caught too. Shape previews are stylised cross-sections — f shown with 3 lobes-pairs as a hint, real shapes are more intricate.

03

Solved Examples (Step-by-Step)

Numbers → legality → counts. Jo chain yahan chalti hai, wahi validator me live chalti hai.

EXAMPLE 01Foundation · NEET

Full profile of n = 4, l = 2

For an electron with n = 4 and l = 2, write the orbital designation, the number of orbitals in the subshell, the electrons it can hold, and its radial and angular nodes.

  1. Legalityl = 2 ≤ n − 1 = 3 ✓ — the orbital exists.
  2. Designationl = 2 → d → 4d (verify on the validator).
  3. Capacityorbitals = 2l + 1 = 5 · electrons = 2(2l + 1) = 10
  4. Nodesradial = n − l − 1 = 1 · angular = l = 2 · total = 3 = n − 1 ✓

4d · 5 orbitals · 10 electrons · 1 radial + 2 angular nodes

EXAMPLE 02JEE Main · Node identity

3s, 3p, 3d — different splits, same total

Compare the radial and angular nodes of 3s, 3p and 3d. What stays constant, and why?

  1. 3sradial = 3 − 0 − 1 = 2 · angular = 0 → 2
  2. 3pradial = 3 − 1 − 1 = 1 · angular = 1 → 2
  3. 3dradial = 3 − 2 − 1 = 0 · angular = 2 → 2
  4. WhyTotal = n − 1 is fixed by the shell; l only re-partitions it between spherical and planar surfaces. A JEE favourite identity ✓

All total 2 nodes — split shifts, sum never

EXAMPLE 03JEE Main · Last electron

The seventh electron of nitrogen

Write the four quantum numbers of the seventh (last) electron of nitrogen (Z = 7), with the rule that decides them.

  1. ConfigurationN: 1s² 2s² 2p³ — the 7th electron lands in 2p.
  2. Hund’s ruleThree degenerate 2p orbitals fill singly with parallel spins first — one electron in each of m = −1, 0, +1.
  3. AssignLast electron (convention: m filled −1 → 0 → +1): n = 2, l = 1, m = +1, s = +½ — the three 2p electrons take m = −1, 0, +1 in turn, so the third one sits in m = +1
  4. Verifyl = 1 ≤ n − 1 ✓ · |m| = 1 ≤ 1 ✓ · Pauli: no clash with the two earlier p electrons (different m) ✓

(2, 1, +1, +½) — Hund’s rule at work

05

Key Formulas & Takeaways

Formula card

Eight lines that solve this topic

Hψ = Eψ · |ψ|² = probability densitySchrödinger’s equation; ψ itself has no physical meaning.
l = 0 … (n − 1)Shape code 0123 = s p d f; subshells per shell = n; kills 1p/2d/3f.
m = −l … +lOrientations per subshell = 2l + 1 (s 1 · p 3 · d 5 · f 7).
Electrons per subshell = 2(2l + 1)s 2 · p 6 · d 10 · f 14 — Pauli allows two per orbital, opposite spins.
Shell: n² orbitals · 2n² electronsn = 3 → 9 orbitals, 18 electrons.
Radial nodes = n − l − 1 · angular = lTotal always n − 1 — the split shifts, the sum is fixed.
Orbital angular momentum = √(l(l+1))·h/2πs 0 · p √2 · d √6 · f √12 — in units of h/2π.
H-like: E ∝ n only · multi-electron: n + lDegeneracy in H; Aufbau order 4s < 3d in multi-electron atoms.

Letters: l = 0, 1, 2, 3 → s, p, d, f  ·  Spin: s = ±½ (experimental)  ·  Orbital size: region of ~90–95% probability  ·  Aufbau ties: equal n + l → lower n fills first (3d before 4p)

  1. Orbital ≠ orbit — a probability cloud from |ψ|² replaced Bohr’s forbidden exact path; that conceptual swap is the model’s core.
  2. Four numbers, one address — n (shell), l (shape, ≤ n−1), m (orientation, |m| ≤ l), s (spin ±½, experimental).
  3. Counts are formulas, not memory — n² orbitals and 2n² electrons per shell; 2l+1 orbitals and 2(2l+1) electrons per subshell; nodes n − l − 1 + l = n − 1.
  4. Two energy universes — hydrogen degenerate within n; multi-electron ordered by n + l, with Aufbau, Pauli and Hund running the filling.
06

FAQs

What are the four quantum numbers and what does each specify?

The principal quantum number n (1, 2, 3, …) fixes the shell — its size and energy. The azimuthal quantum number l (0 to n−1) fixes the subshell shape: 0 is s, 1 is p, 2 is d, 3 is f. The magnetic quantum number m (−l to +l) fixes the orientation of the orbital, giving 2l+1 values. The spin quantum number s (+½ or −½) fixes the electron's intrinsic spin. The first three emerge from solving the Schrödinger equation; spin was added experimentally.

How many orbitals are there in a shell and in a subshell?

A shell with principal quantum number n contains n² orbitals and can hold 2n² electrons. A subshell with azimuthal quantum number l contains 2l+1 orbitals and holds 2(2l+1) electrons — so s holds 2, p holds 6, d holds 10 and f holds 14 electrons.

How do you count radial and angular nodes of an orbital?

Radial (spherical) nodes = n − l − 1, angular (planar) nodes = l, and the total is always n − 1. For example, 3p has 1 radial and 1 angular node (total 2), while 4f has 0 radial and 3 angular nodes (total 3).

What is the difference between an orbit and an orbital?

An orbit is Bohr's fixed circular path where the electron's position and velocity are exact — a picture the uncertainty principle forbids. An orbital is the three-dimensional region around the nucleus where the probability of finding the electron is maximum (about 90–95%), obtained from |ψ|². An orbit is two-dimensional and definite; an orbital is a probability cloud and is the quantum mechanical replacement of the orbit.

04

Practice Questions (With Solutions)

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QCC Notes — Class 11 Chemistry

Strictly NCERT-aligned notes for JEE Main & NEET, prepared by QCC Notes (Padho Likho JEE). Content follows the latest NCERT edition and current NTA exam pattern.

Last updated
24 Sep 2026