Structure of atom

Class 11 · Updated 2026-10-02. Published for practice.

What is inside an atom

An atom is not the final piece. Electrons, protons, and neutrons sit inside it. Other short-lived particles show up in nuclear physics; Class 11 usually sticks to e-, p+, n.

Atomic number Z = number of protons. In a neutral atom, electrons = protons = Z.

Mass number A = protons + neutrons. Neutrons = A − Z.

Isotopes: same Z, different A (same element, different mass). Hydrogen’s common set: 1H, 2H, 3H.

Isobars: same A, different Z (different elements, same mass number). Example pattern: 14C and 14N.

How the particles were found

Cathode rays (discharge tube, low pressure, high voltage): travel straight, deflected toward the positive plate → negative particles. Thomson measured e/m for the electron.

Millikan’s oil-drop work gave the elementary charge scale. The value you write in exams is e ≈ 1.6 × 10-19 C. Use the value your board table prints if they give one.

Anode / canal rays: positive particles; their e/m depends on the gas in the tube. Lightest positive ion from hydrogen → proton.

Neutron: Chadwick (1932). Be bombarded with α-particles → neutral particles with mass close to the proton.

Models you must compare

Thomson (plum pudding): positive sphere with electrons stuck in it. Explains overall neutrality. Fails Rutherford’s scattering results.

Rutherford: most α-particles go straight → mostly empty space. Rare large deflections → tiny, dense, positive nucleus. Electrons outside.

Rutherford’s hole: an orbiting electron should radiate and spiral in (classical EM). Atom would not be stable.

Bohr (for H and one-electron ions): electrons only in allowed orbits; angular momentum mvr = nh/2π; no radiation while in an allowed orbit; jumps between orbits exchange energy as photons.

Bohr works for H-like spectra. It fails multi-electron atoms, fine structure, Zeeman/Stark detail, and it clashes with the uncertainty principle.

Light, photoelectric effect, dual nature

c = νλ. Wave number = 1/λ.

Planck: energy comes in packets. E = hν. h ≈ 6.626 × 10-34 J s (write the value your book uses).

Photoelectric effect: need ν ≥ ν0 (threshold). KE of ejected electron = hν − hν0. Intensity changes how many electrons leave, not their max KE.

de Broglie: matter also has wavelength λ = h/mv = h/p. Useful for electrons; everyday objects have tiny λ, so you do not “see” their wave side.

Heisenberg: you cannot pin exact position and exact momentum of a tiny particle at once. Δx · Δp ≥ h/4π.

Hydrogen line spectrum

Discharge through H2 → line spectrum. Rydberg form: wave number = R(1/n12 − 1/n22), with n2 > n1.

n1 = 2 → Balmer (visible). n1 = 1 → Lyman (UV). Higher series sit further into IR.

R is the Rydberg constant. Use the value printed in your exam data if they give one.

Four quantum numbers

n (principal): shell. Size and energy ladder. n = 1, 2, 3…

l (azimuthal): subshell / shape. l = 0 → s, 1 → p, 2 → d, 3 → f. For a given n, l runs 0 to n−1. Orbitals in a subshell: 2l + 1.

mₗ (magnetic): orientation. For a given l, mₗ = −l … 0 … +l.

mₛ (spin): +1/2 or −1/2.

One orbital holds at most two electrons, opposite spins (Pauli).

Orbital shapes and filling order

s: spherical. p: dumbbell (pₓ, pᵧ, p_z). d: five orbitals (d_xy, d_yz, d_zx, d_x2−y2, d_z2).

Aufbau: fill lower energy first. Common order: 1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p …

(n + l) rule: lower (n + l) fills first; if tied, lower n fills first.

Hund: in a subshell, put one electron in each orbital (same spin) before pairing.

Exam trap: Cr and Cu are exceptions students are expected to know (half-filled / filled d preference). Write Cr: [Ar] 3d5 4s1, Cu: [Ar] 3d10 4s1.

Used in these practicals