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Quantum Theory of Light

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Eventually, the inside will attain the same temperature as the outside. ... A perfect radiator absorbs all radiation falling on it; that is why it is called ... – PowerPoint PPT presentation

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Title: Quantum Theory of Light


1
Quantum Theory of Light
  • Classical Creation Theory

2
Differential Forms
3
Wave Equation
4
Blackbody Radiation
  • Closed Box with a tiny pinhole
  • Inside is heated by emission from the inside
    walls. Eventually, the inside will attain the
    same temperature as the outside.
  • Radiation from the pinhole is called Blackbody
    Radiation
  • A perfect radiator absorbs all radiation falling
    on it that is why it is called a black body.

5
Blackbody Radiation Laws
  • Kirchhoffs Theorem
  • Energy emitted at a frequency f depends only on
    the frequency and the temperature.
  • Stefans Law
  • Total power per unit area emitted at ALL
    frequencies is proportional to the fourth power
    of absolute temperature.

6
Blackbody Radiation Laws
7
Spectral Energy Density
  • We have considered the power radiated per unit
    area per unit frequency J(f,T).
  • Next consider energy per unit volume per unit
    frequency within the Blackbody, u(f,T).
  • The two must be proportional
  • By averaging over direction the constant of
    proportionality is just c/4.

8
Wiens Exponential Law
  • Wein guessed that the universal function u(f,T)
    had the form

9
Plancks Version
  • Plank knew that Weins Law worked fine at short
    wavelengths. He tried to derive the law using
    statistical mechanics and Maxwells Laws.
    Nothing worked.
  • He learned that for long wavelengths that u(f,T)
    was proportional to T.

10
Plancks Version
  • New empirical formula

11
Plancks Version
  • So what is the explanation for h?
  • Billions of resonators in the walls of the
    cavity vibrating at different frequencies
  • Total energy of a resonator could only be an
    integral multiple of hf

12
Plancks Version
  • Resonators at multiple frequencies with emission
    at individual frequencies
  • Equilibrium between resonators and radiation in
    the cavity

13
Plancks Version
  • So, now we have to compute the average energy per
    oscillator
  • Classically, radiation in the cavity is standing
    waves with temperature T
  • According to Boltzmann, average energy must be
    proportional to T for a degree of freedom
  • Compare to ideal gas law!

14
Plancks Version
15
Plancks Version
  • Quantize the energy of the standing waves

16
Plancks Version
17
Plancks Version
  • Assumptions, energynhf
  • Change in energy is hf
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