example of black body spectra for different temperatures

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Page 1: Example of Black Body Spectra for different temperatures
Page 2: Example of Black Body Spectra for different temperatures

Example of Black Body Spectra for different temperatures

Page 3: Example of Black Body Spectra for different temperatures
Page 4: Example of Black Body Spectra for different temperatures

What is the best known example of a black body source?

Page 5: Example of Black Body Spectra for different temperatures

What is the best known example of a black body source? Hint Temperature = 2.7 K

Page 6: Example of Black Body Spectra for different temperatures

Astrophysical Journal, 473, 576

Cosmic Microwave Background (Radiation from Big Bang! T=2.725K. The theoretical curve obscures the data points and the error bars.

Planck Radiation Law

Page 7: Example of Black Body Spectra for different temperatures

Question: What is the energy quantization of a grandfather clock?

Hint:

Page 8: Example of Black Body Spectra for different temperatures

Question: What is the energy quantization of a grandfather clock?

Hint:

E=nhν for n=1, ν=1Hz=1s-1 E= 6.6x10-34J

Page 9: Example of Black Body Spectra for different temperatures

How is the quantization realized?

E=nhν for n=1, ν=1Hz=1s-1 E= 6.6x10-34J

Page 10: Example of Black Body Spectra for different temperatures

How does this quantization translate into quantization of the pendulum displacement (height)?

E=nhν for n=1, ν=1Hz=1s-1 E= 6.6x10-34J

Page 11: Example of Black Body Spectra for different temperatures

How does this quantization translate into quantization of the pendulum displacement (height)?

E=nhν for n=1, ν=1Hz=1s-1 E= 6.6x10-34J

E=mgH=6.6x10-34J H=6.6x10-34J/(1kg 10m/s2)=6.6x10-35m H

Too small to measure (size of an atom is about 10-8 m)

Page 12: Example of Black Body Spectra for different temperatures

Configuration Prediction (Classical)

Observation

Brighter Light

Very Bright Red Light

Change Color

Time until emission of electricity

Metal

Page 13: Example of Black Body Spectra for different temperatures

Configuration Prediction (Classical)

Observation

Brighter Light More Electricity Faster electrons

Very Bright Red Light

More Electricity

Change Color No Effect

Time until emission of electricity

Few Seconds Metal

Page 14: Example of Black Body Spectra for different temperatures

Configuration Prediction (Classical)

Observation

Brighter Light More Electricity Faster electrons

YES NO

Very Bright Red Light

More Electricity No electricity

Change Color No Effect Big Effect

Time until emission of electricity

Few Seconds

Instantaneous (~10-9 s) Metal

Page 15: Example of Black Body Spectra for different temperatures

Robert Millikan 1868-1953 Nobel Prize in Physics 1923

"for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect"

"for his work on the elementary charge of electricity and on the photoelectric effect"

Albert Einstein 1879-1955 Nobel Prize in Physics 1921

Max Planck 1858-1947 Nobel Prize in Physics 1918

Emission and Absorption of Light evidence for quantization

"in recognition of the services he rendered to the advancement of Physics by his discovery of energy quanta".

Page 16: Example of Black Body Spectra for different temperatures

Diagram of Millikan’s Device For measuring photoelectric effect

Page 17: Example of Black Body Spectra for different temperatures

Data from Millikan’s 1916 Article

Page 18: Example of Black Body Spectra for different temperatures

Phys. Rev. 7, 355–388 (1916)

Page 19: Example of Black Body Spectra for different temperatures

Example Problem The work functions for K and Zn are 2.26 eV and 4.24 eV Which will emit photoelectrons when illuminated by Red, Blue and UV light?

Wavelength K (2.26 eV) Zn (4.24 eV)

Red (700 nm)

Blue (400 nm)

UV (280 nm)

E=hν-w=0 hc=1240eV nm Energy of photon is hν or hc/λ or 1240 eV nm/ λ

Page 20: Example of Black Body Spectra for different temperatures

Example Problem The work functions for K and Zn are 2.26 eV and 4.24 eV Which will emit photoelectrons when illuminated by Red, Blue and UV light?

Wavelength K (2.26 eV) Zn (4.24 eV)

Red (700 nm)

Blue (400 nm)

UV (280 nm)

E=hν-w=0 hc=1240eV nm Energy of photon is hν or hc/λ or 1240 eV nm/ λ

? Photon Photoelectron? E= hc/λ If (hc/λ− w) > 0

Page 21: Example of Black Body Spectra for different temperatures

Example Problem The work functions for K and Zn are 2.26 eV and 4.24 eV Which will emit photoelectrons when illuminated by Red, Blue and UV light?

E=hν-w=0 hc=1240eV nm Energy of photon is hν or hc/λ or 1240 eV nm/ λ

? Photon Photoelectron? E= hc/λ If (hc/λ− w) > 0

Wavelength K (2.26 eV) Zn (4.24 eV)

Red (700 nm) 1.77 eV NO NO

Blue (400 nm) 3.10 eV YES NO

UV (280 nm) 4.42 eV YES YES

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