Ratio of energy densities of black body radiation

In summary, the conversation discussed the correct formula for energy density and simplified it to show that it corresponds to option (B).
  • #1
Pushoam
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Homework Statement


upload_2017-12-31_14-4-30.png


Homework Equations

The Attempt at a Solution

The energy density is given as ## u = \frac { 8 \pi {\nu }^2}{c^3}~ \frac { h \nu} {e^{ \frac { h\nu}{k_B T}} – 1}.##

EDIT : I put the constant C.
## \frac { u( 2 \nu) } {u(\nu)} = C \frac { {e^{ \frac { h\nu}{k_B T}} – 1} }{ {e^{ \frac { 2h\nu}{k_B T}} – 1} } ##
Where C is the appropriate constant.

Is this correct?
 

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  • #2
Pushoam said:

Homework Statement


View attachment 217649

Homework Equations

The Attempt at a Solution

The energy density is given as ## u = \frac { 8 \pi {\nu }^2}{c^3}~ \frac { h \nu} {e^{ \frac { h\nu}{k_B T}} – 1}##.

## \frac { u( 2 \nu) } {u(\nu)} = \frac { {e^{ \frac { h \nu}{k_B T}} – 1} }{ {e^{ \frac { 2h \nu}{k_B T}} – 1} } ##

Is this correct?
The formula is correct (apart from a constant factor), but you have to simplify it and figure out which option it corresponds to. Note that ##e^{ \frac { 2h \nu}{k_B T}}=\left(e^{ \frac { h \nu}{k_B T}}\right)^2##
 
  • #3
ehild said:
Note that ##e^{ \frac { 2h \nu}{k_B T}}=\left(e^{ \frac { h \nu}{k_B T}}\right)^2##

Thanks for this insight.
## \frac { u( 2 \nu) } {u(\nu)} = \frac { {e^{ \frac { h\nu}{k_B T} } – 1} } { \left ({e^{ \frac { h\nu}{k_B T}} – 1}\right ) \left( {e^{ \frac { h\nu}{k_B T}} +1} \right) } ## ## = \frac1 {e^{ \frac { h\nu}{k_B T}} +1} ##

So, the answer is option (B).
 
Last edited:
  • #4
Pushoam said:
Thanks for this insight.
## \frac { u( 2 \nu) } {u(\nu)} = \frac { {e^{ \frac { h\nu}{k_B T} } – 1} } { \left ({e^{ \frac { h\nu}{k_B T}} – 1}\right ) \left( {e^{ \frac { h\nu}{k_B T}} +1} \right) } ## ## = \frac1 {e^{ \frac { h\nu}{k_B T}} +1} ##

So, the answer is option (B).
Yes :)
 

Related to Ratio of energy densities of black body radiation

1. What is the ratio of energy densities of black body radiation?

The ratio of energy densities of black body radiation is a measure of the distribution of electromagnetic radiation emitted by a black body at different wavelengths. It is represented by the symbol "u" and is equal to the energy density at a given wavelength divided by the energy density at the peak wavelength of the black body.

2. How is the ratio of energy densities of black body radiation calculated?

The ratio of energy densities of black body radiation can be calculated using the Planck's law, which describes the spectral energy density of electromagnetic radiation emitted by a black body. The equation for calculating the ratio is u(λ)/u(λmax) = (2hc^2/λ^5) / (exp(hc/λkT) - 1), where h is the Planck's constant, c is the speed of light, k is the Boltzmann constant, T is the temperature in Kelvin, λ is the wavelength, and λmax is the peak wavelength of the black body.

3. What does the ratio of energy densities of black body radiation tell us?

The ratio of energy densities of black body radiation is an important quantity in understanding the behavior of black bodies. It tells us the relative amount of energy emitted by a black body at different wavelengths, which is essential in determining the color and temperature of the black body. It also helps in studying the properties of matter and the nature of radiation.

4. How does the ratio of energy densities of black body radiation change with temperature?

The ratio of energy densities of black body radiation changes with temperature because the peak wavelength of the black body shifts towards shorter wavelengths as the temperature increases. This results in a decrease in the ratio at longer wavelengths and an increase at shorter wavelengths. This phenomenon is known as Wien's displacement law.

5. How is the ratio of energy densities of black body radiation related to the Stefan-Boltzmann law?

The ratio of energy densities of black body radiation is related to the Stefan-Boltzmann law, which states that the total energy radiated by a black body is proportional to the fourth power of its absolute temperature. This means that as the temperature of a black body increases, the ratio of energy densities also increases, indicating a higher energy output at all wavelengths. This relationship helps in understanding the amount of energy emitted by a black body and its dependence on temperature.

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