Trouble understanding the idea of a cavity radiator being a Black Body

In summary, the conversation discusses the role of a cavity as a black body radiator in the derivation of Planck's black body radiation law. The main questions raised include the behavior of perfect absorbers and emitters, the effect of external heat sources on radiation, and the formation of standing waves due to boundary conditions. The experts provide helpful resources and clarify that the Bose factor and average occupation number are more accurate representations of the energy and states of a mode, rather than equating to kT.
  • #1
kal
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1
I have been trying to understand the role of a cavity as a black body radiator in the derivation of planks black body radiation law but it has left me with 5 main questions:

1. If an object is a perfect absorber it must also be a perfect emitter, meaning that (allowing for a cavity not being a perfect representation) most of the light that enters the cavity should come back out through the hole. But given the size of the hole compared to the cavity won't most of the radiation escape through the walls and barely any through the hole.

2. if the cavity is being kept at a constant temperature by an external heat source won't this heat permeate the walls and add to the radiation inside the cavity so that it isn't all energy from the light entering the cavity?

3. Apparently the electric field of the wave must be 0 at the walls of the cavity but I don't understand the reasoning.

4. how does the boundary condition that the electric field must be 0 at the walls lead to the formation of standing waves?

5. When deriving planks law for blackbody radiation it calculates the density of modes inside the cavity as a function of frequency, assuming that all modes at that frequency are filled. Why is it the case that all the modes must be filled and is that still the case for cavities at a low temperature?

Any help would be much appreciated :)

I understand why the a ray of light that enters the cavity has little chance of getting out and therefore must be absorbed, making the hole and cavity a near perfect absorber. I also understand from a thermodynamics point of view that if in thermal equilibrium it must be a perfect emitter.

My first question is what is the physical reason for why the cavity and hole is a perfect emitter? (e.g for being a perfect absorber it was that the radiation can't escape)

My second is what does being a perfect emitter even mean because a perfect absorber absorbs all radiation that hits it but all objects will eventually radiate away all their heat.

Thanks in advance :)
 
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  • #2
In the derivation of the Planck function, (5) is incorrect. The average occupation number is given by the Bose factor ## \bar{n}_s=\frac{1}{e^{E_s/kT}-1} ##. In addition, I don't think (3) is necessary in the derivation. The derivation I like best is the one in F.Reif, Statistical and Thermal Physics. To count the cavity modes, you simply assume periodic boundary conditions. ## \\ ## See also post 206 of this rather lengthy thread: https://www.physicsforums.com/threads/emission-spectra-of-different-materials.913274/page-11 Also see the "link" in post 208 of this same thread for counting the modes: To repeat that "link" here: https://www.physicsforums.com/threads/boltzmann-vs-maxwell-distribution.918232/ See in particular, posts 2 and 4 to count the modes.
 
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  • #3
Charles Link said:
In the derivation of the Planck function, (5) is incorrect. The average occupation number is given by the Bose factor ## \bar{n}_s=\frac{1}{e^{E_s/kT}-1} ##. In addition, I don't think (3) is necessary in the derivation. The derivation I like best is the one in F.Reif, Statistical and Thermal Physics. To count the cavity modes, you simply assume periodic boundary conditions. ## \\ ## See also post 206 of this rather lengthy thread: https://www.physicsforums.com/threads/emission-spectra-of-different-materials.913274/page-11 Also see the "link" in post 208 of this same thread for counting the modes: To repeat that "link" here: https://www.physicsforums.com/threads/boltzmann-vs-maxwell-distribution.918232/ See in particular, posts 2 and 4 to count the modes.
My undersanding was that ##\frac{8\pi \nu^2}{c^3}## was the possible number of states of a certain frequency and that ##h\nu## multiplied by the bose-einstien factor was the quantum equivalent to KT the average energy since that is what it approximates too. Is this wrong?
 
  • #4
kal said:
My undersanding was that ##\frac{8\pi \nu^2}{c^3}## was the possible number of states of a certain frequency and that ##h\nu## multiplied by the bose-einstien factor was the quantum equivalent to KT the average energy since that is what it approximates too. Is this wrong?
I believe the result that "this equates to kT " is a high temperature result of the Bose factor for ## kT>>E_s ##. The Bose factor is correct regardless of the energy of the mode.
 
  • #5
Charles Link said:
I believe the result that "this equates to kT " is a high temperature result of the Bose factor for ## kT>>E_s ##. The Bose factor is correct regardless of the energy of the mode.
aha okay thanks a bunch, those links were also very helpful :)
 
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  • #6
Charles Link said:
In the derivation of the Planck function, (5) is incorrect. The average occupation number is given by the Bose factor ## \bar{n}_s=\frac{1}{e^{E_s/kT}-1} ##. In addition, I don't think (3) is necessary in the derivation. The derivation I like best is the one in F.Reif, Statistical and Thermal Physics. To count the cavity modes, you simply assume periodic boundary conditions. ## \\ ## See also post 206 of this rather lengthy thread: https://www.physicsforums.com/threads/emission-spectra-of-different-materials.913274/page-11 Also see the "link" in post 208 of this same thread for counting the modes: To repeat that "link" here: https://www.physicsforums.com/threads/boltzmann-vs-maxwell-distribution.918232/ See in particular, posts 2 and 4 to count the modes.
One more thing, ## \frac{1}{e^{E_s/kT}-1} ## asymptotes with the x axis, so if this is the average occupancy of a state won't all states be occupied since the function never equals 0
 
  • #7
kal said:
One more thing, ## \frac{1}{e^{E_s/kT}-1} ## asymptotes with the x axis, so if this is the average occupancy of a state won't all states be occupied since the function never equals 0
For low temperatures and high energies, the denominator gets quite large, making ## \bar{n}_s ## very small. ## \bar{n}_s ## is the average occupancy number. That number may be .000001 or less for a mode where ## E_s>> kT ##. It never goes precisely to zero, but can be very near zero.
 
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  • #8
I think the reason has to do with the fact that when the radiation is confined to an enclosure, the occupancy of the modes of the electromagnetic waves is always at their thermal equilibrium value of ## \bar{n}_s=\frac{1}{e^{E_s/kT}-1} ##. e.g. A gas in free space at that temperature that occupies the same volume as the enclosure will in general have a very low emissivity, and the thermal motion of the particles, coupled to the E-M waves (E-M modes), simply isn't able to supply the energy to keep the EM states occupied, unless the gas is confined to an enclosure. As soon as an E-M mode gets some energy, in the form of photons, the photons travel at the speed of light away from the gas, and those photons are gone. ## \\ ## With some solids, and also with ionized gases, the emissivity is generally higher, and in some cases emissivities can be nearly 1.0. In the case of ionized gases and solids, there can be considerably more coupling between the thermal motion of the particles and the modes of the electromagnetic waves. (The occupancy number ## n_s ## value can be maintained closer to the equilibrium value with more coupling). ## \\ ## The enclosure with a small aperture is the best way though of getting an emissivity that is very nearly 1.0. ## \\ ## Additional item is if you make the aperture too large, you will no longer have emissivity equal to 1.0. This can also be seen from Kirchhoff's law, where some of the energy incident on the aperture will enter the enclosure and reflect back out, if the aperture is not very small. ## \\ ## Perhaps someone else has a better explanation, but this is how I understand it. ## \\ ## And to answer your second question, you do need to supply heat to your ideal blackbody source that is radiating energy away in order to keep it at the same temperature, so it can continue to radiate at that temperature.
 
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  • #9
kal said:
My first question is what is the physical reason for why the cavity and hole is a perfect emitter? (e.g for being a perfect absorber it was that the radiation can't escape)
That is not the right conclusion. Any incident radiation will be absorbed because it will not be reflected but the inside will still have a temperature and radiate in its own right. The rate of emission will be equal to the rate of absorption when the inside and (effective) outside temperatures are equal. 'Obviously' there can be no overall build up of energy in the cavity beyond the equilibrium condition.
 
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  • #10
The most clear derivation of the Planck law in the 21st century is to use thermal QED. Of course, as always in statistics of gases you have to use a finite quantization volume and then take the infinite-volume limit in the correct physical way. You find this derivation in my unfinished manuscript on photons:

https://th.physik.uni-frankfurt.de/~hees/pf-faq/photon.pdf
 

1. What is a cavity radiator?

A cavity radiator is any object with a hollow or enclosed space that can emit or absorb electromagnetic radiation. This can include objects such as a light bulb, a laser, or a microwave oven.

2. What is a Black Body?

A Black Body is an idealized object that absorbs and emits all radiation that falls on it. It does not reflect or transmit any radiation, and therefore appears black in color. It is used as a theoretical model to understand the properties of radiation and how it interacts with matter.

3. How does a cavity radiator behave like a Black Body?

A cavity radiator behaves like a Black Body because the enclosed space inside the cavity allows for multiple reflections of radiation, leading to a uniform distribution of energy. This makes the radiation emitted by the cavity radiator closely resemble the spectrum of a Black Body.

4. Why is it important to understand the concept of a cavity radiator as a Black Body?

Understanding the behavior of a cavity radiator as a Black Body is important in many scientific fields, such as thermodynamics, astronomy, and materials science. It allows us to accurately predict and measure the emission and absorption of radiation, which has practical applications in fields such as energy production and climate science.

5. Can a real-life object ever behave exactly like a Black Body?

No, a real-life object can never behave exactly like a Black Body. While some objects, such as stars, can closely resemble a Black Body, there will always be some deviations due to factors like surface properties and imperfections. However, the concept of a Black Body serves as a useful tool for understanding and analyzing radiation in various applications.

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