1. Electron emission and the photoelectric effect
- Work function : least energy needed to free an electron from a metal surface; 1 eV = 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 : . Different intensities, same ν: different saturation currents, same .
- Frequency: same intensity, higher ν: same saturation current, larger . against ν is a straight line cutting the axis at the threshold frequency ; slope for all metals.
- No time lag (< s).
- Wave theory fails: it predicts rising with intensity, emission at any frequency, and a time lag in dim light.
- photocurrent ∝ intensity (ν > ν₀)
- intensity I₁
- intensity 2I₁
- intensity 3I₁
- ν₁
- ν₂ > ν₁
- ν₃ > ν₂
Formulas
- Stopping potential
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: , , speed , zero rest mass, no charge. Intensity ∝ number of photons per second (for one frequency). J s; eV nm.
- One photon is absorbed by one electron: , i.e. .
- Threshold: , .
- : slope (same for all metals), intercept (depends on the metal).
- Explains: independent of intensity; threshold; linear rise with ν; instant emission; current ∝ number of photons.
- potassium (φ₀ = 2.25 eV, ν₀ = 5.43 × 10¹⁴ Hz)
- zinc (φ₀ = 4.3 eV, ν₀ = 10.38 × 10¹⁴ Hz)
Formulas
- Einstein’s photoelectric equation
- Photon energy
- Threshold wavelength
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 has wavelength .
- Charged particle accelerated through : , ; electron: nm.
- Equal kinetic energy: . Equal momentum: equal .
- Everyday objects: far too small to observe; electrons: comparable to atomic spacings (basis of the electron microscope).
- electron: λ = 1.227/√V nm
Formulas
- de Broglie relation
- Electron accelerated through V
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 ), I–V at different frequencies (same saturation).
- ; slope of –ν is .
- eV nm; 1 eV = J.
- ; electron nm.