Equation of state of photon gas

In summary, the conversation is about using the stress-energy tensor to derive the equation of state of a photon gas. The person has completed all steps except for finding the average value of [cos(θ)]^2 over a unit sphere. They have tried integrating over the sphere but have not been successful. Another person suggests changing variables and integrating from 0 to 2π on φ and -1 to +1 on μ to get the total area. Then, using this, they can solve for the average value of [cos(θ)]^2 which turns out to be 1/3.
  • #1
4everphysics
19
0
Dear all,

I am using stress-energy tensor to derive equation of state of photon gas (assuming it as a perfect fluid).
I completed all the steps except one:

average value of [cos(θ)]^2 over unit sphere = 1/3.

I have no idea how this is so. (θ is polar angle).
I tried integrating over 0<θ<∏ and 0<φ<2∏, and then divided by the surface area of the sphere, but no luck with that either...

Please help!
 
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  • #2
The element of surface area on a sphere is sin θ dθ dφ. Thus if you integrate this over the entire sphere, ∫∫sin θ dθ dφ you should get the total area.

Change variables to μ = cos θ and integrate from 0 to 2π on φ and -1 to +1 on μ.

∫∫ dμ dφ = (2)(2π) = 4π, the total area.

Now for your integral,

∫∫ μ2 dμ dφ = 2π [1/3 μ3]-11 = 4π/3. Divide this by the total area and you get 1/3.
 

Related to Equation of state of photon gas

1. What is the equation of state of photon gas?

The equation of state of photon gas describes the relationship between the pressure, volume, and temperature of a gas composed entirely of photons, such as electromagnetic radiation. It is given by the equation P = ρ/3, where P is the pressure, ρ is the energy density, and c is the speed of light.

2. How is the equation of state of photon gas derived?

The equation of state of photon gas can be derived from the ideal gas law by considering the energy density of photons as the product of their number density and their average energy per photon, which is given by Planck's law. By substituting this into the ideal gas law and using the fact that photons have no mass, the equation of state can be derived.

3. What are the assumptions made in the equation of state of photon gas?

The equation of state of photon gas is based on the assumption that the gas is in thermal equilibrium and that the photons are traveling at the speed of light. It also assumes that the photons are not interacting with each other or any other particles, and that the gas is composed entirely of photons.

4. How does the equation of state of photon gas differ from that of a classical gas?

The equation of state of photon gas differs from that of a classical gas in several ways. Firstly, the equation only applies to a gas composed of photons, while the classical gas equation applies to any gas. Additionally, the pressure of a photon gas is directly proportional to its energy density, while the pressure of a classical gas is directly proportional to its number density.

5. What is the significance of the equation of state of photon gas?

The equation of state of photon gas has significant implications in fields such as astrophysics, cosmology, and high-energy physics. It can be used to study the behavior of radiation in the early universe and in extreme conditions, such as in the cores of stars. It also plays a crucial role in understanding the properties of light and electromagnetic radiation in various environments.

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