List I (n, l, mₗ)
List II (Orbital)
Quick Rules: n = shell, l→subshell (0=s,1=p,2=d,3=f), orbital name = n + subshell letter
| n, l, mₗ | l→subshell | mₗ valid? | Orbital |
|---|---|---|---|
| A: 3,0,0 | 0→s | 0 to 0 ✓ | 3s = IV ✓ |
| B: 4,1,0 | 1→p | −1 to +1 ✓ | 4p = I ✓ |
| C: 3,2,1 | 2→d | −2 to +2 ✓ | 3d = III ✓ |
| D: 4,2,−2 | 2→d | −2 to +2 ✓ | 4d = II ✓ |
Every electron in an atom is uniquely described by four quantum numbers. The Pauli Exclusion Principle states no two electrons can have the same set of all four quantum numbers. Together they define the energy, shape, orientation, and spin of each electron's orbital.
n → Principal quantum number → 1, 2, 3, 4... (shell)
l → Azimuthal quantum number → 0 to (n−1) (subshell shape)
mₗ → Magnetic quantum number → −l to +l (orbital orientation)
ms → Spin quantum number → +½ or −½ only
📌 l = 0 → s subshell → spherical → 1 orbital (mₗ = 0 only)
📌 l = 1 → p subshell → dumbbell → 3 orbitals (mₗ = −1, 0, +1)
📌 l = 2 → d subshell → cloverleaf → 5 orbitals (mₗ = −2 to +2)
📌 l = 3 → f subshell → complex → 7 orbitals (mₗ = −3 to +3)
📌 Number of orbitals in subshell l = 2l + 1
📌 Max electrons in subshell = 2(2l + 1)
The quantum numbers are not independent — each must satisfy strict constraints. For a given n: l can be 0, 1, 2... up to (n−1). For a given l: mₗ can be −l, −l+1, ... 0, ... l−1, +l (total 2l+1 values). ms is always +½ or −½ regardless of n, l, or mₗ. A quantum number set is invalid if l ≥ n or |mₗ| > l. For example, (2,2,0) is invalid because for n=2, l can only be 0 or 1, not 2.
| n (shell) | Subshells (l) | Total orbitals | Max e⁻ |
|---|---|---|---|
| 1 (K) | 1s | 1 | 2 |
| 2 (L) | 2s, 2p | 4 | 8 |
| 3 (M) | 3s, 3p, 3d | 9 | 18 |
| 4 (N) | 4s, 4p, 4d, 4f | 16 | 32 |
Orbitals fill in order of increasing (n + l). When two subshells have the same (n + l), the one with lower n fills first. The correct filling order: 1s → 2s → 2p → 3s → 3p → 4s → 3d → 4p → 5s → 4d → 5p → 6s → 4f → 5d → 6p. This explains why 4s fills before 3d — 4s has n+l=4 while 3d has n+l=5.
Pauli Exclusion: maximum 2 electrons per orbital, with opposite spins. This limits s-subshell to 2 electrons, p to 6, d to 10, f to 14. Hund's Rule: electrons fill degenerate orbitals one each with parallel spins before pairing begins. This maximises total spin and gives the most stable configuration. For carbon (1s²2s²2p²): the two 2p electrons are in separate 2p orbitals with parallel spins, not both in the same orbital.
Chromium (Cr, Z=24): Expected [Ar]3d⁴4s², Actual [Ar]3d⁵4s¹. The half-filled 3d⁵ configuration (all five 3d orbitals singly occupied with parallel spins) has extra stability due to maximum exchange energy and spherical electron distribution. Copper (Cu, Z=29): Expected [Ar]3d⁹4s², Actual [Ar]3d¹⁰4s¹. The completely filled 3d¹⁰ subshell is extra stable. These are the most commonly tested exceptions in NEET.
When electrons transition between energy levels, photons are emitted or absorbed. The energy of emitted photon: E = 13.6(1/n₁² − 1/n₂²) eV for hydrogen. Different series correspond to different final states: Lyman series (n₁=1, UV), Balmer (n₁=2, visible), Paschen (n₁=3, IR), Brackett (n₁=4, IR), Pfund (n₁=5, far IR). The Balmer series (H-alpha at 656 nm etc.) gives the visible colours of hydrogen discharge tubes.