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Dual Nature of Radiation and Matter — Notes

4 sections 3 min readBeta

1. Electron emission and the photoelectric effect

  • Work function φ0\varphi_0: least energy needed to free an electron from a metal surface; 1 eV = 1.6×10−191.6 \times 10^{-19} J. Emission by heat (thermionic), strong field (field emission) or light (photoelectric).
  • Hertz (1887): ultraviolet light helped sparks across a gap. Hallwachs: a negatively charged zinc plate discharged in UV; a neutral plate became positive. Lenard: UV on the emitter of an evacuated tube produced a current that stopped when the light was cut off; the particles were electrons (photoelectrons).
  • Zinc and cadmium need UV; alkali metals (Na, K, Cs) respond to visible light.

Key terms

Work function

Minimum energy needed to remove an electron from the surface of a metal.

Photoelectric effect

Emission of electrons from a surface when light of suitable frequency falls on it.

2. Experimental study

Emitter C and collector A in an evacuated tube; light through a quartz window; collector potential variable and reversible; microammeter for the photocurrent.

  • Intensity: photocurrent ∝ intensity (number of electrons per second ∝ intensity).
  • Potential: current rises to a saturation value as A is made positive; it falls to zero at the stopping potential −V0-V_0: eV0=KmaxeV_0 = K_\text{max}. Different intensities, same ν: different saturation currents, same V0V_0.
  • Frequency: same intensity, higher ν: same saturation current, larger V0V_0. V0V_0 against ν is a straight line cutting the axis at the threshold frequency ν0\nu_0; slope h/eh/e for all metals.
  • No time lag (< 10−910^{-9} s).
  • Wave theory fails: it predicts KmaxK_\text{max} rising with intensity, emission at any frequency, and a time lag in dim light.
  • photocurrent ∝ intensity (ν > ν₀)
  • intensity I₁
  • intensity 2I₁
  • intensity 3I₁
Same frequency: saturation current ∝ intensity; stopping potential unchanged.
  • ν₁
  • ν₂ > ν₁
  • ν₃ > ν₂
Same intensity: higher frequency, larger stopping potential.

Formulas

  • Stopping potential
    eV0=Kmax=12mvmax2eV_0 = K_\text{max} = \tfrac{1}{2}m v_\text{max}^2

Key terms

Stopping potential

The negative collector potential that just stops the most energetic photoelectrons; eV₀ = K_max.

Threshold frequency

Minimum frequency of light that can cause photoelectric emission from a given metal.

Saturation current

Maximum photocurrent, reached when all emitted electrons are collected.

3. Photons and Einstein’s photoelectric equation

  • Light is a stream of photons: E=hν=hc/λE = h\nu = hc/\lambda, p=h/λp = h/\lambda, speed cc, zero rest mass, no charge. Intensity ∝ number of photons per second (for one frequency). h=6.63×10−34h = 6.63 \times 10^{-34} J s; hc≈1240hc \approx 1240 eV nm.
  • One photon is absorbed by one electron: hν=φ0+Kmaxh\nu = \varphi_0 + K_\text{max}, i.e. Kmax=eV0=hν−φ0=h(ν−ν0)K_\text{max} = eV_0 = h\nu - \varphi_0 = h(\nu - \nu_0).
  • Threshold: ν0=φ0/h\nu_0 = \varphi_0/h, λ0=hc/φ0\lambda_0 = hc/\varphi_0.
  • V0=heν−φ0eV_0 = \dfrac{h}{e}\nu - \dfrac{\varphi_0}{e}: slope h/eh/e (same for all metals), intercept ν0\nu_0 (depends on the metal).
  • Explains: KmaxK_\text{max} independent of intensity; threshold; linear rise with ν; instant emission; current ∝ number of photons.
Drawn to scale for 400 nm light on potassium (φ₀ = 2.25 eV).
  • potassium (φ₀ = 2.25 eV, ν₀ = 5.43 × 10¹⁴ Hz)
  • zinc (φ₀ = 4.3 eV, ν₀ = 10.38 × 10¹⁴ Hz)
Slope h/e is the same for every metal; the intercept on the ν axis is the threshold frequency ν₀ = φ₀/h.

Formulas

  • Einstein’s photoelectric equation
    Kmax=hν−φ0=eV0K_\text{max} = h\nu - \varphi_0 = eV_0
  • Photon energy
    E=hν=hcλE = h\nu = \dfrac{hc}{\lambda}
  • Threshold wavelength
    λ0=hcφ0\lambda_0 = \dfrac{hc}{\varphi_0}

Key terms

Photon

A quantum of electromagnetic radiation with energy hν and momentum h/λ.

4. Matter waves

  • Dual nature: radiation shows wave (interference, diffraction) and particle (photoelectric effect) behaviour.
  • de Broglie relation: a particle of momentum pp has wavelength λ=hp=hmv=h2mK\lambda = \dfrac{h}{p} = \dfrac{h}{mv} = \dfrac{h}{\sqrt{2mK}}.
  • Charged particle accelerated through VV: K=qVK = qV, λ=h2mqV\lambda = \dfrac{h}{\sqrt{2mqV}}; electron: λ≈1.227V\lambda \approx \dfrac{1.227}{\sqrt{V}} nm.
  • Equal kinetic energy: λ∝1/m\lambda \propto 1/\sqrt{m}. Equal momentum: equal λ\lambda.
  • Everyday objects: λ\lambda far too small to observe; electrons: comparable to atomic spacings (basis of the electron microscope).
  • electron: λ = 1.227/√V nm
λ = h/√(2meV) ≈ 1.227/√V nm.

Formulas

  • de Broglie relation
    λ=hp=h2mK\lambda = \dfrac{h}{p} = \dfrac{h}{\sqrt{2mK}}
  • Electron accelerated through V
    λe≈1.227V nm\lambda_e \approx \dfrac{1.227}{\sqrt{V}}\ \text{nm}

Key terms

de Broglie wavelength

Wavelength associated with a moving particle, λ = h/p.

Exam tips

  • Three graphs: I–intensity (line), I–V at different intensities (same −V0-V_0), I–V at different frequencies (same saturation).
  • eV0=Kmax=hν−φ0eV_0 = K_\text{max} = h\nu - \varphi_0; slope of V0V_0–ν is h/eh/e.
  • hc≈1240hc \approx 1240 eV nm; 1 eV = 1.6×10−191.6 \times 10^{-19} J.
  • λ=h/p=h/2mK\lambda = h/p = h/\sqrt{2mK}; electron 1.227/V1.227/\sqrt{V} nm.