Weins Displacement Law: Calculating Max Wavelength & Frequency

In summary, Wien's Displacement Law is a physical law that relates the wavelength of the peak emission of a black body to its temperature. It states that the product of the peak wavelength and the absolute temperature of the black body is a constant value. The maximum wavelength can be calculated by dividing the constant value of 2.8977729 x 10^-3 meters-kelvin by the temperature in Kelvin. This gives the peak wavelength in meters. However, it can only be applied to objects that emit thermal radiation, such as stars or heated objects. It cannot be applied to objects that do not emit thermal radiation, such as non-heated objects or objects at very low temperatures. The maximum frequency can be calculated by dividing the speed of
  • #1
pseudo
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in weins displacement law how can we calculate the maximum wavelength & the maximum frequency? is that equation applicable for all kinds of black body radiations even the hawking radiation ?
 
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  • #2
Wavelength and frequency are linked via [itex] c=f\lambda[/itex]. As far as I know it should be applicable to Hawking radiation as well.
 
  • #3


Wein's Displacement Law is a fundamental principle in physics that relates the maximum wavelength of radiation emitted by a black body to its temperature. This law states that the product of the maximum wavelength and the temperature of a black body is a constant, known as Wien's constant (denoted by the symbol "b"). Mathematically, this can be written as λmaxT = b.

To calculate the maximum wavelength, we can rearrange the equation to solve for λmax, which gives us λmax = b/T. Similarly, to calculate the maximum frequency, we can use the relationship between wavelength and frequency, which is given by the equation c = νλ, where c is the speed of light. Rearranging this equation to solve for the frequency (ν), we get ν = c/λ. Therefore, the maximum frequency can be calculated as νmax = c/λmax = c/(b/T) = T/b.

This equation is applicable for all kinds of black body radiations, including Hawking radiation. Hawking radiation is a type of thermal radiation predicted to be emitted by black holes due to quantum effects near the event horizon. While it is not a traditional black body radiation, it still follows Wein's Displacement Law as it is based on the temperature of the black hole.

In conclusion, Wein's Displacement Law is a powerful tool for understanding the relationship between temperature and the maximum wavelength and frequency of radiation emitted by black bodies. It can be applied to all types of black body radiations, including Hawking radiation. By using this law, we can gain a deeper understanding of the properties and behavior of various forms of radiation in the universe.
 

Related to Weins Displacement Law: Calculating Max Wavelength & Frequency

1. What is Wien's Displacement Law?

Wien's Displacement Law is a physical law that relates the wavelength of the peak emission of a black body to its temperature. It states that the product of the peak wavelength and the absolute temperature of the black body is a constant value.

2. How is the maximum wavelength calculated using Wien's Displacement Law?

The maximum wavelength can be calculated by dividing the constant value of 2.8977729 x 10^-3 meters-kelvin by the temperature in Kelvin. This gives the peak wavelength in meters.

3. Can Wien's Displacement Law be applied to all objects?

Wien's Displacement Law can only be applied to objects that emit thermal radiation, such as stars or heated objects. It cannot be applied to objects that do not emit thermal radiation, such as non-heated objects or objects at very low temperatures.

4. How is the maximum frequency calculated using Wien's Displacement Law?

The maximum frequency can be calculated by dividing the speed of light (3 x 10^8 meters per second) by the peak wavelength calculated using Wien's Displacement Law. This gives the peak frequency in Hertz.

5. What is the significance of Wien's Displacement Law in astrophysics?

Wien's Displacement Law is used in astrophysics to determine the temperature of stars and other celestial objects. By measuring the peak wavelength of their thermal radiation, scientists can calculate the temperature of these objects, providing valuable information about their composition and evolution.

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