Atoms

Physics · Class 12

Lesson 12 of 12 · 14 min

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Must-know facts

18 facts

  1. 01Thomson (1898): plum pudding model, positive charge spread through the atom with electrons embedded.
  2. 02Geiger–Marsden (about 1911): 5.5 MeV alpha-particles from ²¹⁴₈₃Bi on gold foil 2.1 × 10⁻⁷ m thick; ZnS screen and microscope.
  3. 03About 0.14% scattered by more than 1°; about 1 in 8000 by more than 90°.
  4. 04Nucleus 10⁻¹⁵ to 10⁻¹⁴ m; atom about 10⁻¹⁰ m, 10,000 to 100,000 times larger.
  5. 05Small impact parameter → large scattering; head-on (b smallest) → rebound, θ ≈ π.
  6. 06Closest approach d = 2Ze²/(4πε₀K); 7.7 MeV alpha on gold: d = 3.0 × 10⁻¹⁴ m = 30 fm; gold radius about 6 fm.
  7. 07Gold: Z = 79, about 50 times heavier than an alpha-particle.
  8. 08Hydrogen orbit: r = e²/(4πε₀mv²); E = −e²/(8πε₀r); K = −E, U = 2E.
  9. 09Ground state: r = 5.3 × 10⁻¹¹ m, v = 2.2 × 10⁶ m/s, E = −13.6 eV.
  10. 10Classical revolution frequency in hydrogen's ground orbit: about 6.6 × 10¹⁵ Hz.
  11. 11Bohr: stationary orbits, L = nh/2π, hν = Ei − Ef.
  12. 12rn ∝ n², vn ∝ 1/n, En = −13.6/n² eV = −2.18 × 10⁻¹⁸/n² J.
  13. 13E₂ = −3.40 eV, E₃ = −1.51 eV; excitation 10.2 eV (1→2) and 12.09 eV (1→3).
  14. 14Ionisation energy of hydrogen: 13.6 eV; n = ∞ has E = 0; continuum above E = 0.
  15. 15Absorption lines fall at the same wavelengths as the gas's emission lines.
  16. 16de Broglie (1923): 2πrn = nλ gives mvr = nh/2π; Davisson–Germer confirmed electron waves in 1927.
  17. 17Bohr model works only for hydrogenic atoms (H, He⁺, Li²⁺) and cannot give line intensities.
  18. 18Bohr received the Nobel Prize in Physics in 1922.

Common traps

Where marks are lost

Formulas

9 to know

Coulomb force on the alpha-particle

F = (1/4πε₀)(2e)(Ze)/r²

Z = 79 for gold.

Distance of closest approach

d = 2Ze²/(4πε₀K)

Head-on; K is the alpha-particle's kinetic energy.

Orbit radius and speed

r = e²/(4πε₀mv²)

From mv²/r = e²/(4πε₀r²).

Energy of the orbiting electron

E = −e²/(8πε₀r)

K = −E, U = 2E.

Bohr's quantisation

L = mvr = nh/2π

n = 1, 2, 3 …

Photon from a transition

hν = Ei − Ef

Absorption: Ei + hν = Ef.

Radius of the nth orbit

rn = (n²/m)(h/2π)²(4πε₀/e²)

rn = n²a₀, a₀ = 5.3 × 10⁻¹¹ m.

Energy of the nth level

En = −me⁴/(8n²ε₀²h²) = −13.6/n² eV

= −2.18 × 10⁻¹⁸/n² J.

Standing-wave condition

2πrn = nλ

With λ = h/mv this gives mvr = nh/2π.

Key terms

15 terms

Plum pudding model
Thomson's atom: positive charge spread through the whole atom, electrons embedded in it.
Nuclear model
Rutherford's atom: all the positive charge and most of the mass in a tiny central nucleus.
Scintillation
A brief flash of light when an alpha-particle strikes a zinc sulphide screen.
Impact parameter
Perpendicular distance of an alpha-particle's initial velocity line from the centre of the nucleus.
Scattering angle
The angle θ between the alpha-particle's initial and final directions.
Distance of closest approach
Separation at which a head-on alpha-particle momentarily stops before turning back.
Emission line spectrum
Bright lines at specific wavelengths on a dark background, from an excited rarefied gas.
Absorption spectrum
Dark lines in a continuous spectrum at the wavelengths a gas absorbs.
Stationary state
An allowed orbit in which the electron does not radiate and the atom has a definite energy.
Principal quantum number
The integer n labelling Bohr's orbits and energy levels.
Bohr radius
Radius of hydrogen's innermost orbit, a₀ = 5.3 × 10⁻¹¹ m.
Ground state
The lowest-energy state, n = 1; −13.6 eV for hydrogen.
Excited state
Any state with n > 1, reached by collisions or by absorbing a photon.
Ionisation energy
Least energy to free the electron from the ground state: 13.6 eV for hydrogen.
Hydrogenic atom
A nucleus of charge +Ze with one electron, such as H, He⁺ or Li²⁺.
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Atoms Revision Notes | Class 12 Physics NCERT