Black Body and Radiation Spectrum
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Black Body and Radiation Spectrum

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Questions and Answers

What is a black body?

A black body is a perfect absorber and radiator of radiation.

A perfect black body exists in nature.

False

Who devised a black body that approximates closely to the properties of a perfect black body?

Fery

Fery's black body consists of a metallic cavity in the form of a double walled hollow copper sphere with a ___ coating from inside.

<p>lamp black</p> Signup and view all the answers

What happens to the radiation falling on the hole in Fery's black body?

<p>It is absorbed with multiple reflections.</p> Signup and view all the answers

What is the radiation coming out of a black body when heated at constant temperature called?

<p>Black body radiation</p> Signup and view all the answers

What was the focus of the experiments conducted by Lummer and Pringsheim between 1893 to 1897?

<p>Energy distribution in black body radiation spectrum</p> Signup and view all the answers

According to Stefan's Law, what is the relationship between the area under the curve of radiation energy and the fourth power of the absolute temperature?

<p>The area is directly proportional to the fourth power of the absolute temperature.</p> Signup and view all the answers

What does Wien's displacement law state about the wavelength corresponding to maximum energy?

<p>It shifts to the shorter wavelength side as the temperature increases.</p> Signup and view all the answers

What did Max Planck propose in 1900 regarding radiation?

<p>Energy is emitted in discrete packets called quanta.</p> Signup and view all the answers

What is the formula for the energy values of Planck's oscillator?

<p>En = nhv</p> Signup and view all the answers

In the average energy of Planck’s oscillator, E is calculated as E = ΣE/N, where N is the total number of ___ .

<p>oscillators</p> Signup and view all the answers

What is the Planck constant represented by?

<p>h</p> Signup and view all the answers

Study Notes

Black Body

  • A black body is a perfect absorber and radiator of electromagnetic radiation

  • A black body does not exist in nature, but Fery’s black body is a good approximation

  • Fery's black body design:

    • A double-walled hollow copper sphere
    • Coated with lamp black on the inside and nickel polished on the outside
    • A narrow conical hole acts as an entry and exit point
    • A projection within the cavity prevents radiation from escaping
    • The space between the walls is evacuated to minimize heat loss
  • Fery's black body acts as a perfect absorber:

    • Incoming radiation undergoes multiple reflections before escaping, ensuring full absorption
  • Fery's black body acts as a perfect radiator:

    • When heated to a constant temperature, it emits blackbody radiation

Blackbody Radiation Spectrum

  • Lummer and Pringsheim experimented with blackbody radiation from 1893 to 1897

  • They measured the energy distribution of the spectrum using:

    • A heated hollow enclosure acting as a blackbody
    • A thermocouple to measure the blackbody's temperature
    • Concave mirrors to direct the radiation
    • A fluorspar prism to disperse the radiation into a spectrum
    • A bolometer to detect the radiation intensity at different wavelengths
  • Key observations:

    • Energy distribution in the spectrum is not uniform
    • Energy intensity rises with wavelength, reaches a maximum, and then decreases
    • Total energy emitted at a given temperature is proportional to the fourth power of the absolute temperature (Stefan's Law)
    • The peak wavelength (wavelength corresponding to maximum energy) shifts to shorter wavelengths as the temperature increases (Wien's Displacement Law)
  • Existing theoretical formulas, like Wien's and Rayleigh-Jeans, couldn't fully explain the experimental blackbody radiation curves

Planck’s Quantum Hypothesis

  • Max Planck proposed his radiation law in 1900

  • Planck's assumptions:

    • The cavity contains oscillators of molecular dimensions vibrating at different frequencies
    • These oscillators emit and absorb radiation at their own frequencies
    • Oscillators can only exchange energy in discrete packets called quanta (photons)
    • The energy of a quantum is dependent on the oscillator's frequency: E = hv, where h is Planck's constant
  • Planck's explanation:

    • Oscillators have discrete energy levels: En = nhv (n = 0, 1, 2, 3,...), where n is an integer
    • Energy exchange is limited to multiples of hv (0, hv, 2hv, 3hv, ..., nhv)

Average Energy of Planck's Oscillator

  • N is the total number of oscillators
  • E is the total energy
  • The average energy is: E = ΣE / N
  • No, N1, N2, Nr, ... represent the number of oscillators with energies 0, hv, 2hv, ... nhv
  • The number of oscillators with energy rhv is: Nr = No e-rholky
  • The total number of oscillators is: N = No + N1 + N2 + ...

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Description

Explore the concepts of black bodies and blackbody radiation through this quiz. Learn about Fery's black body design, its properties, and the historical experiments conducted by Lummer and Pringsheim. Test your understanding of how black bodies absorb and emit electromagnetic radiation.

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