Planck's Radiation Law and Stefan's Law

In summary, the conversation discusses two questions related to the derivation of Planck's Radiation Law and Stefan's Law. The first question addresses the assumption of standing waves in the derivation of Planck's Radiation Law and why only standing waves are considered. This is due to Maxwell's boundary conditions at an interface, which state that the electric field must be continuous across the interface. The second question asks about the application of thermodynamics in studying radiation and why it behaves like a gas. The answer is that radiation occupies a finite space and exerts finite pressure, allowing for the application of thermodynamics. The conversation concludes with the person finding the answer to their questions and sharing it with others.
  • #1
manofphysics
41
0
I have got 2 questions:
1)In the derivation of Planck's Radiation Law,we assume an enclosure of perfectly reflecting walls which contains diffuse radiations.These are EM waves which reflect from the walls.
Now, in my book(or even http://thermalhub.org/topics/DerivationofPlancksLaw"), it is further said that standing waves are formed which limit the wavelength to
[tex]\lambda=2l/n_{i}[/tex].
Now why are ONLY standing waves formed ?Any type of wave can be formed after reflection from the walls.Why are taking the assumption that displacement at the end of walls is zero?

2)In the derivation of Stefan's Law as given by Boltzmann, why can we apply all the thermodynamic relation and thermodyanamic laws ? Does radiation behave exactly like a gas?
I know that pressure of diffuse radiation is similar to that exerted by a ideal gas, but I STILL can't understand how and why thermodyanmics is used in radiations?
 
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  • #2
I am disappointed . No reply after over 200 views.

I found out the answer myself.For all the people who didn't know,

1)This is due to Maxwell's boundary conditions at an interface.
[tex]E_{1}^{||}-E_{2}^{||}=0[/tex]
where [tex]E_{1}, E_{2}[/tex] represent fields in air and conductor respectively.

2)As radiation occupies a finite space and exerts finite pressure, and hence can do work,
So we can apply thermodynamics in this case.
 
  • #3



1) The assumption of perfectly reflecting walls and diffuse radiation is made in the derivation of Planck's Radiation Law in order to simplify the problem and make it more manageable. Standing waves are formed because they are the only type of wave that can exist in a confined space, such as an enclosure with reflecting walls. This is due to the boundary conditions at the walls, where the displacement must be zero in order to satisfy the requirement of perfect reflection. While other types of waves may be formed after reflection, they would not be able to exist in this confined space due to the boundary conditions. Therefore, standing waves are the only solution that can exist in this scenario.

2) In the derivation of Stefan's Law, we apply thermodynamic relations and laws because radiation behaves similarly to a gas in some ways. Just like a gas, radiation has properties such as temperature, pressure, and energy. Thermodynamics is used to understand and describe the behavior of radiation in terms of these properties. While radiation may not behave exactly like a gas, the principles and laws of thermodynamics can still be applied to understand its behavior. This allows us to make predictions and calculations about radiation, such as in the case of Stefan's Law which relates the energy emitted by a blackbody to its temperature.
 

FAQ: Planck's Radiation Law and Stefan's Law

What is Planck's Radiation Law?

Planck's Radiation Law is a fundamental law of physics that describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature. It states that the energy of the radiation emitted by a black body is directly proportional to the frequency of the radiation and inversely proportional to the temperature of the body.

Who discovered Planck's Radiation Law?

Max Planck, a German physicist, discovered Planck's Radiation Law in 1900 while studying the properties of black body radiation. He proposed that electromagnetic energy is quantized, meaning it can only exist in discrete packets of energy called "quanta". This theory revolutionized the understanding of energy and laid the foundation for the development of quantum mechanics.

What is Stefan's Law?

Stefan's Law, also known as the Stefan-Boltzmann Law, is a fundamental law of physics that relates the amount of energy emitted by a black body to its temperature. It states that the total energy emitted per unit surface area per unit time by a black body is directly proportional to the fourth power of its absolute temperature.

How are Planck's Radiation Law and Stefan's Law related?

Planck's Radiation Law and Stefan's Law are closely related as they both describe the properties of black body radiation. Planck's Law describes the spectral distribution of the radiation, while Stefan's Law describes the total amount of energy emitted by a black body. Together, these laws provide a comprehensive understanding of the behavior of black body radiation.

What are the practical applications of Planck's Radiation Law and Stefan's Law?

Planck's Radiation Law and Stefan's Law have many practical applications in fields such as astronomy, astrophysics, and engineering. These laws are used to calculate the energy output of stars and other celestial bodies, design and optimize thermal systems, and understand the behavior of various materials at high temperatures. They are also essential for the development of new technologies, such as solar panels and infrared cameras.

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