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.
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- (J s)
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- (Hz)
- (m)
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- (m)
- (K)
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- (W/(m² K⁴))
- (m²)
- (K)
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- (J)
- (C)
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- (rad)
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- (kg)
- (m/s)
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- (J s)
- (kg m/s)
- (kg)
- (m/s)
Constant used
Given
- (J s)
- (m)
- (kg m/s)
Constant used
Given
- (J s)
- (J)
- (s)
Constant used