Undergrad Equilibrium between objects at different temperatures?

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The discussion revolves around a thought experiment involving two black bodies in a vacuum at 0 K, where radiation from one body is focused onto the other. Participants question the feasibility of such an optical system, citing the conservation of etendue and thermodynamic laws, particularly the zeroth and second laws. They argue that if the bodies reach thermal equilibrium, they must have the same temperature, contradicting the initial assumption of differing temperatures. The conversation also touches on the implications of thermal conductors and the complexities of radiation transfer in such a setup. Ultimately, the consensus is that the original assumptions about the optical device are flawed, leading to contradictions in thermodynamic principles.
  • #31
It seems to me that an attempt to eschew Thermodynamics in this description is misguided because of complexity. For instance there is no requirement that the emission from the surface is isotropic. It is more likely to be Lambertian, but such details cannot matter in the bigger picture. So better to think of the black body cavity as a "gas of photons" at a temperature T corresponding to that of the "container". In fact any chunk of ordinary matter is more or less such a partition, and hence the ubiquity of tha Stefan-Boltzmann Law.
In the concentric spherical case by symmetry one can deal easily with the problem posed in the original post. The equilibrium state is T=0 for everything. If instead you supply power P, then the steady state depends upon $$ P=4\pi R^2\sigma (T^4-0)$$ for the outer shell. If you supply the power only to the inner sphere it will be warmer than the outer shell according to its area .
 
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  • #32
hutchphd said:
It seems to me that an attempt to eschew Thermodynamics in this description is misguided because of complexity. For instance there is no requirement that the emission from the surface is isotropic. It is more likely to be Lambertian, but such details cannot matter in the bigger picture. So better to think of the black body cavity as a "gas of photons" at a temperature T corresponding to that of the "container". In fact any chunk of ordinary matter is more or less such a partition, and hence the ubiquity of tha Stefan-Boltzmann Law.
In the concentric spherical case by symmetry one can deal easily with the problem posed in the original post. The equilibrium state is T=0 for everything. If instead you supply power P, then the steady state depends upon $$ P=4\pi R^2\sigma (T^4-0)$$ for the outer shell. If you supply the power only to the inner sphere it will be warmer than the outer shell according to its area .
I have to add something.
The whole construction is isolated from the rest of the universe so no radiation or heat can escape by any means.
I'm not supplying any power anywhere so the only thing the sphere and the inner wall of the cavity can do is settle into a static equilibrium.

I agree that I maybe shouldn't assume isotropic emission from the cavity wall, but it's the simplest model and I wonder if that detail could make such a big difference.
Or maybe that's exactly what's wrong.
 
  • #33
hutchphd said:
For instance there is no requirement that the emission from the surface is isotropic. It is more likely to be Lambertian, ....
According to Wikipedia it's supposed to be isotropic: https://en.wikipedia.org/wiki/Black_body

That might not be trustworthy, of course.
 
  • #34
Hi. This is interesting topic.
Even without some special lenses or fiber optics the dilemma is there.

I also made my own calculations and can confirm yours.

For example, if r=1 and R=2 then,
small sphere receives 13.4% of big sphere's thermal radiation,
while for temperatures to remain same it needs to receive 25%.
So, big sphere's temperature will settle higher than small sphere's.

If you consider Lambertian radiation,
this means a surface point equivalently radiates to a lesser solid angle than 2*pi.
Let's check correction factor to 13.4% and to other radii:

for r=1 and R=2 it is 25/13.4= 1.8656

r=1 and R=1.001 gives ratio of 1.045
r=1 and R=1.01 gives ratio of 1.14
r=1 and R=1.1 gives ratio of 1.4166
r=1 and R=2 gives ratio of 1.8656
r=1 and R=3 gives ratio of 1.9425
r=1 and R=4 gives ratio of 1.9685

Seems ratio goes from 1(when radii are almost equal), to 2(when radii ratio is very big).
Which is expected because in Lambertian, a point radiates much more to up than sides.
And when small sphere occupies small solid angle "above" a point on big sphere,
the difference is biggest.

Maybe Lambertian is the solution to the dilemma, or maybe not.

These are calculations, hope there are no mistakes.
I follow this topic to see how this dilemma will be solved.
 
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  • #35
jonhswon said:
I follow this topic to see how this dilemma will be solved.
Me too.

Maybe the whole approach of comparing outgoing and incoming radiation is wrong, but why?
 
  • #36
This is indeed much more interesting than one (me, in particular) might expect at first glance. The etendu theorem is really a statement about a sort of "optical free energy" (my colloquial term), considering both energy and entropy. The theorem's requirement that etendu cannot passively decrease is the second law of thermodynamics for a beam of light. Attempts to show it using energy conservation alone cannot be viable. Thanks for the question @Philip Koeck
 
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  • #37
A quick update on whether or not radiation from a black body is isotropic.

I've read a bit about Lambert's law in an old book (Optical Physics by Max Garbuny) and he mentions that a glowing sphere looks like a flat disk, which means that radiation from the surface of a black body is actually isotropic.
If radiation was more intense in the direction orthogonal to the surface the sphere would look like a disk that fades out towards its edge.

The brightness (or radiance), however, is proportional to the cosine of the angle (measured from the direction orthogonal to the surface). (This is Lambert's law.)
This is simply because brightness is given as power per solid angle and per emitting area.
 
  • #38
Here is how Walter Greiner presents it in Quantum Mechanics: An Introduction:
1694698857141.png

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1694698870664.png

1694698889428.png

1694698896880.png

1694698902839.png
 
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  • #39
DrClaude said:
Greiner and Garbuny use the word radiance for different things, I think.

Anyway, if I read Greiner correctly, a detector of fixed area placed inside a hot black body cavity will detect the same power no matter where it is placed and in what direction it is facing.

Does that sound right?

That's in principle what I assumed in my calculation from a previous post.
 
  • #40
Philip Koeck said:
Greiner and Garbuny use the word radiance for different things, I think.

Anyway, if I read Greiner correctly, a detector of fixed area placed inside a hot black body cavity will detect the same power no matter where it is placed and in what direction it is facing.

Does that sound right?

That's in principle what I assumed in my calculation from a previous post.
I think I have to correct that.
Right now I believe I assumed that the radiation coming from a given surface element of fixed size on the cavity is isotropic, and that is not right. That should actually follow Lambert's law.
That would change my derivation quite a lot.
I have to think a bit more about that.
 
  • #41
Philip Koeck said:
I think I have to correct that.
Right now I believe I assumed that the radiation coming from a given surface element of fixed size on the cavity is isotropic, and that is not right. That should actually follow Lambert's law.
That would change my derivation quite a lot.
I have to think a bit more about that.
Good news: If I take into account that radiation power per solid angle emitted from a fixed surface element is proportional to cos φ, where φ is the angle measured from the direction perpendicular to the surface, then the fraction f from post 30 is actually given by sin2a and therefore TS=TC.

A connected question: Does Lambert's law follow only from the second law or is there some other way to show it?
 
  • #42
You need to specify a particular derivation if you desire meaningful commentary. This is very difficult to follow. There are a number of ways to state Lambert's Law(s) for instance.
 
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  • #43
Philip Koeck said:
A connected question: Does Lambert's law follow only from the second law or is there some other way to show it?
I invoke the Anna Karenina principle here and direct you to a paper by Zhang
 
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  • #44
hutchphd said:
You need to specify a particular derivation if you desire meaningful commentary. This is very difficult to follow. There are a number of ways to state Lambert's Law(s) for instance.
To start with here's the calculation I discussed in post 30 with the correction to a brightness that's proportional to cos φ.
Sorry for the quality of the image. It looks good when I open the file on my computer, but it get's fuzzy when I upload it.

This text shows that this angular dependence of radiation (what I call Lambert's law) is in agreement with the second law.

I'll send another, more direct, argument for Lambert's law when I get round to it.

Radiationequilibrium2.jpg
 
  • #45
In the restframe of the black-body radiation it's homogeneous and isotropic. If it were not, there'd be heat flow from some parts of the container walls to others through radiation until thermal equilibrium is reached.

Lambert's cosine Law follows from this. It's however not about the distribution of black-body radiation within the cavity, which is homogeneous and isotropic in its rest frame, but about the radiation of a black body to the outside. It describes the energy flow of radiation from a surface, and the cosine is that of the angle between the emitter's surface normal and the direction of observation. The Wikipedia is pretty good, as far as I can see:

https://en.wikipedia.org/wiki/Lambert's_cosine_law
 
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  • #46
vanhees71 said:
In the restframe of the black-body radiation it's homogeneous and isotropic. If it were not, there'd be heat flow from some parts of the container walls to others through radiation until thermal equilibrium is reached.

Lambert's cosine Law follows from this. It's however not about the distribution of black-body radiation within the cavity, which is homogeneous and isotropic in its rest frame, but about the radiation of a black body to the outside. It describes the energy flow of radiation from a surface, and the cosine is that of the angle between the emitter's surface normal and the direction of observation. The Wikipedia is pretty good, as far as I can see:

https://en.wikipedia.org/wiki/Lambert's_cosine_law
I'll skip my own thought experiment, since it's essentially the same as what's discussed in the Wikipedia page shared by vanHees71 and also in the sections from Greiner shared by DrClaude (plus some other sources).

The argument for the cosine law is that it's necessary to make radiation isotropic and homogeneous and that, in turn, is necessary for two bodies (or parts of the same surface) to be in equlibrium at equal temperatures.

So you could say that the second law requires Lambert's law.

Is there any other way to show that the cosine law has to hold?
 
  • #47
That there must be this cosine in the calculation of how much radiation energy flows through a surface is very general. It's just the definition of the "energy-current density". As for any current density, the em. field energy going through an arbitrary given surface per unit time is
$$\int_S \mathrm{d}^2 \vec{f} \cdot \vec{S},$$
where ##\vec{S} \propto \vec{E} \times \vec{B}## is the Poynting vector. The cosine is hidden, of course, in the scalar product between the Poynting vector and the surface-normal vector under the intgral.
 
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  • #48
vanhees71 said:
That there must be this cosine in the calculation of how much radiation energy flows through a surface is very general. It's just the definition of the "energy-current density". As for any current density, the em. field energy going through an arbitrary given surface per unit time is
$$\int_S \mathrm{d}^2 \vec{f} \cdot \vec{S},$$
where ##\vec{S} \propto \vec{E} \times \vec{B}## is the Poynting vector. The cosine is hidden, of course, in the scalar product between the Poynting vector and the surface-normal vector under the intgral.
I'm not sure whether that's really what I'm looking for.

Clearly there must be a cosine factor for radiation that flows through a surface, but what about radiation that's emitted from a surface.

Why is the power per solid angle and emitting surface not independent of the angle?
 
  • #49
I think thermal radiation lambertian emission pattern is how nature works, and so is the related law of thermo. Is there a need to establish which one gives birth to the other? They just work together.

Isotropic pattern is unrealistic/wrong, but combined with such a wrong view factor that in the end it yields correct result, it works. Like (-1)*(-1)=1.

edit: added the word "thermal radiation"
 
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  • #50
jonhswon said:
I think lambertian emission pattern is how nature works, and so is the related law of thermo. Is there a need to establish which one gives birth to the other? They just work together.
Radiation from an electric dipole, for example, is not lambertian.

I would say things that happen in nature are in agreement with the 2nd law, but that doesn't mean they are caused by the 2nd law.

Heat is never completely converted to work (without also producing waste heat) simply because this extremely unlikely. The 2nd law simply states that such an unlikely event will usually not happen. It doesn't cause it not to happen.

I think some other reason for Lambert's law would be interesting.
At the moment we only have: "It has to be like that in order to agree with the 2nd law."
 
  • #51
I meant thermal radiation pattern emitted from a surface being lambertian is natural. :)
 
  • #52
jonhswon said:
I meant thermal radiation pattern emitted from a surface being lambertian is natural. :)
Yes, I know you meant that, but I'm wondering what causes it to be lambertian.

The 2nd law doesn't qualify as a cause of things. It only tells you what cannot happen, but it doesn't actually do a good job predicting what will happen.

You can think of the following process:
You place a lump of metal on a metal surface. Then you add heat to the metal lump and suddenly the lump starts gliding along the surface and some waste heat is transferred to the metal surface.

As long as the amount of waste heat is large enough the 2nd law has no problem with this process, but that doesn't mean it will happen.

In this example you see that 2nd law doesn't tell you what's going to happen, simply because it has nothing to do with mechanisms.

All things that happen do so in agreement with the 2nd law, but not because of it.

That's my view anyway.
 
  • #53
Philip Koeck said:
By some ingenious optical device all the radiation from body 1 is focused onto body 2 and vice versa.

Philip Koeck said:
Me too.

Maybe the whole approach of comparing outgoing and incoming radiation is wrong, but why?
I think the apparent paradox is to do with the assumption that the two bodies only exchange energy. I thought about a perfect ellipsoid (already discussed) and my conclusion was that a single object at one focus would only be radiating and receiving energy from itself. That would be an equilibrium situation. Put a minute object at the other focus. It only takes up a small part of the image of the larger object so it cannot interact with it all and its equilibrium temperature would be reached when the energy received equalled the energy emitted. The small object would be an exact equivalent of a small part (same area) of the large object. Stefan's law says this will happen when the added object is at the same temperature as the original object. Stefan's law assumes / implies that the object under discussion only radiates outwards and ignores the above situation.

The same argument applies for a small object inside a big one. The effective area of the inside of the big one is actually the same as the area of the small one inside. All the energy that's unaccounted for is passing between the parts of the internal face of the outside one.
 
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  • #54
sophiecentaur said:
The same argument applies for a small object inside a big one. The effective area of the inside of the big one is actually the same as the area of the small one inside. All the energy that's unaccounted for is passing between the parts of the internal face of the outside one.
In post 44 I shared a (visually rather fuzzy) calculation for a spherical black object (arbitrary diameter as long as it fits) in the center of a spherical black cavity.
The result is that the two surfaces will be in equilibrium at equal temperature if (and, I believe, only if) radiation given off from a surface is proportional to cos a, where a is the angle with respect to the surface's normal.
Without the cosine dependence I don't get equilibrium at equal temperatures.
It seems that the cosine-dependence is actually essential for the 2nd law to hold.
 
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  • #55
Philip Koeck said:
It seems that the cosine-dependence is actually essential for the 2nd law to hold.
That's interesting. If the object inside is reduced in size to be just a tiny (infinitessimal) 'probe', you'd expect it to measure the temperature of the inside face of the big hole. If the internal object / probe were almost to fit entirely within the big object then, again, it would be at the same temperature.
Choose an intermediate size and could there be any argument that the inside object could be at a higher or lower temperature and what sort of curve would result as the inner object expanded or contracted?
That implies (and cross checks?) that your cos dependence would have to apply.
 
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  • #56
sophiecentaur said:
That's interesting. If the object inside is reduced in size to be just a tiny (infinitessimal) 'probe', you'd expect it to measure the temperature of the inside face of the big hole. If the internal object / probe were almost to fit entirely within the big object then, again, it would be at the same temperature.
Choose an intermediate size and could there be any argument that the inside object could be at a higher or lower temperature and what sort of curve would result as the inner object expanded or contracted?
That implies (and cross checks?) that your cos dependence would have to apply.
So far the only argument for this cos-dependence (Lambert's law) I've seen is that it's required by the second law.
People have also argued that it's natural, but I can only see that for absorption, not for emission, unless I again say it's required by the second law.

What I'm looking for now is some other explanation for Lambert's law, for example based on the emission properties of optical phonons.
 
  • #57
A cos pattern in the vertical plane is what you get from a horizontal transmitting dipole, λ/r4 above the ground. Thinking in terms of EM theory, it seems to me that currents flowing randomly across the surface of a radiator (in all directions) could produce a radiation distribution which follows Lambert's Law. The maxes and nulls in the horizontal plane would average out to half.

Is that crazy, do you think?
1695909075594.png
 
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  • #58
sophiecentaur said:
A cos pattern in the vertical plane is what you get from a horizontal transmitting dipole, λ/r4 above the ground. Thinking in terms of EM theory, it seems to me that currents flowing randomly across the surface of a radiator (in all directions) could produce a radiation distribution which follows Lambert's Law. The maxes and nulls in the horizontal plane would average out to half.

Is that crazy, do you think?View attachment 332745
Just to clarify. Is the model that there are currents and maybe dipole oscillation mainly in the plane of the surface, but otherwise in random orientations?
This would mean that each "donut" of radiation has a maximum in the direction normal to the plain.
Now these donuts actually have a sin2-profile, but due to the random in-plane orientations this could average out to a cos-profile.
Could work!

I'm not quite sure how you would get zero for a direction parallel to the surface, though.

What does the sin2-donut give when you rotationally average it?

Just to explain why I'm discussing this: It would be interesting that the cos-behaviour of black-body radiation follows from some other physics and then actually agrees with the second law.
That would be like other physics "adapting" to the 2nd law, in a way.
 
  • #59
sophiecentaur said:
A cos pattern in the vertical plane is what you get from a horizontal transmitting dipole, λ/r4 above the ground.
Maybe you could explain this once more. What is the vertical plane and what do you mean by λ/r4 above the ground?
 
  • #60
Philip Koeck said:
Maybe you could explain this once more. What is the vertical plane and what do you mean by λ/r4 above the ground?
Sorry; a typo. I meant λ/4. Different heights will produce different vertical patterns and my choice of λ/4 was a bit arbitrary but the radiation in the horizontal direction will always be equal if the induced ground image is assumes to be perfect. This link shows patterns of dipoles at different heights. The common feature is a zero elevation. A random selection of independent dipole (uncorrelated signals) will (?) have a max 90 degrees and a null at 0 degrees.
The 'vertical plane' would be the vertical plane through the maximum in the horizontal direction. A large number of dipoles, radiating uncorrelated signals in random azimuths will average out as omnidirectional.

The snag here is that a vertical dipole / monopole will have a maximum at zero elevation. I don't know about the orientation of molecular dipoles on the surface of a solid. Maybe horizontal is a fanciful choice.
 
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