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NSMQ

Introduction to Quantum Physics

Classical physics lost this argument in three separate places and each loss pointed the same way. The light from a hot object refused to follow the curve theory predicted, unless the energy of the vibrating charges came in whole bundles. Light falling on a clean metal surface would free electrons, but only if its frequency was high enough, however bright it was. And X-rays bounced off electrons as though they were particles, losing exactly the energy a particle collision would cost them. The blocks work through those three results in order, then follow the compromise that settled the matter, that every particle also has a wavelength and that position and momentum cannot both be pinned down at once.

Quantized energy of a radiating oscillator

Given

  • (J s)
  • (Hz)

Constant used

Energy of a single photon

Given

  • (J s)
  • (Hz)
  • (m)

Constants used

Wien's displacement law for a blackbody

Given

  • (m)
  • (K)
Stefan's law for the power radiated by a hot body

Given

  • (W/(m² K⁴))
  • (m²)
  • (K)

Constant used

Maximum kinetic energy of an emitted photoelectron

Given

  • (J s)
  • (Hz)
  • (J)

Constant used

Threshold frequency for the photoelectric effect

Given

  • (J)
  • (J s)

Constant used

Stopping potential in a photoelectric experiment

Given

  • (J)
  • (C)

Constant used

Momentum of a photon

Given

  • (J)
  • (m)

Constants used

Compton shift in the wavelength of a scattered photon

Given

  • (rad)
  • (kg)

Constants used

Compton wavelength of an electron

Given

  • (J s)
  • (kg)
  • (m/s)

Constants used

de Broglie wavelength of a particle

Given

  • (J s)
  • (kg m/s)
  • (kg)
  • (m/s)

Constant used

Heisenberg uncertainty principle for position and momentum

Given

  • (J s)
  • (m)
  • (kg m/s)

Constant used

Heisenberg uncertainty principle for energy and time

Given

  • (J s)
  • (J)
  • (s)

Constant used

The Nature of Electromagnetic Waves
The Double-Slit Experiment Revisited
A New Model: The Quantum Particle