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NSW HSC Physics (Year 12) · Module 7 The Nature of Light · 25 questions · 50 minutes
Planck's revolutionary idea was that energy is quantised: an oscillator can only emit or absorb whole packets . This discreteness suppresses high-frequency emission and resolved the ultraviolet catastrophe.
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Classical theory predicted the emitted intensity would rise without limit as the wavelength got shorter (into the UV), which is impossible. Planck's quantisation suppressed high-frequency emission and matched the observed curve.
Wien's law: .
By Wien's law a shorter peak wavelength means a higher temperature. A hotter black body's curve lies above the cooler one at every wavelength, so it is both hotter and brighter overall.
Emission requires , i.e. a frequency above the threshold . Below no electrons escape however bright the light; above it, even dim light ejects electrons immediately.
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More intensity means more photons per second, so more electrons per second (a larger current). But each electron's depends only on frequency, so its maximum KE is unchanged.
The retarding voltage does work against the electrons. At the stopping voltage even the fastest electrons are turned back and the current falls to zero, so .
. The photon's energy is split between freeing the electron (the work function) and the electron's kinetic energy.
At threshold , so .
. Then (green). Longer wavelengths cannot eject electrons.
, so . With expressed in eV the stopping voltage in volts is numerically equal: .
Photon energy . Then .
Wien's law gives . Halving the peak wavelength doubles the temperature.
Emission needs the photon energy to exceed . Red (no); green (yes); UV (yes). Intensity is irrelevant to whether emission occurs.
. At double the frequency , which exceeds by . Because of the offset, is not proportional to , so doubling more than doubles it.
Rearranged, . So the gradient is (the same for every metal), the x-intercept is the threshold frequency , and the y-intercept is .
The gradient is . Then .
. With : .
Twice the intensity means twice as many photoelectrons per second, so the saturation current doubles. But , and hence , depends only on the frequency, so the stopping voltage is unchanged (both curves cut the axis at the same ).
Energy per photon . Photons per second .
The wave model predicts that a bright enough beam of any frequency should eventually free electrons (after a delay), with more KE for brighter light. Experiment shows a sharp threshold frequency, instantaneous emission and , all explained by photons of energy . Reflection, interference, polarisation and refraction are the wave model's successes.
. From : .
Photon energy at : . Work function . Longest wavelength is the threshold: .
HSC physics exam skills and the move through senior science to go alongside the practice.
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