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1 Historically Significant Experiments Blackbody Radiation Ultraviolet Catastrophe (Raleigh, Jeans) Planck’s solution Lesson: Energy is not continuous but is

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Published by , 2016-02-14 05:36:02

Historically Significant Experiments

1 Historically Significant Experiments Blackbody Radiation Ultraviolet Catastrophe (Raleigh, Jeans) Planck’s solution Lesson: Energy is not continuous but is

Historically Significant
Experiments

Blackbody Radiation

Ultraviolet Catastrophe (Raleigh, Jeans)
Planck’s solution
Lesson: Energy is not continuous but is

quantized
Planck’s constant h was
introduced

Photoelectric effect

Hertz (1886)
Einstein’s solution (1905)
Lesson: Light has a

corpuscular/particle character
Introduced the concept of a
Photon
Photon has energy E=hν=hc/λ

1

Compton effect

Lesson: Light has a
corpuscular/particle character
and linear momentum p=h/λ

DeBroglie Wavelength

Lesson: Particles have a wavelength
λ=h/p

Davisson, Germer

2

Atomic spectra are not continuous
(line spectra)

Balmer
Rydberg
Explained by Bohr theory
Lesson: Angular momentum of electron

in atom is quantized
In multiples of h

Heisenberg Uncertainty Principle

Lesson: Cannot know the location of a
particle with absolute precision
∆x∆p>h/2π

3


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