Blackbody Radiation: Exploring Beyond \nu

In summary: I'm asking.The easy way is to say that the mode with the same frequency as the resonator is, albeit abstract, just another harmonic oscillator, so the average energy at a given temperature should be the same.
  • #1
dEdt
288
2
I have a quick question about blackbody radiation.

Planck modeled a blackbody as a collection of harmonic oscillators. Then he assumed that each oscillator could only have a energy [itex]E[/itex] equal to [itex]nh\nu[/itex], where [itex]\nu[/itex] is the frequency of the oscillator.

My question is, how can a collection of oscillators like this ever emit radiation which does not have frequency [itex]\nu[/itex] as well?
 
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  • #2
dEdt said:
My question is, how can a collection of oscillators like this ever emit radiation which does not have frequency [itex]\nu[/itex] as well?

It's a collection of harmonic oscillators of different frequencies; all the frequencies are represented.
 
  • #3
Nugatory said:
It's a collection of harmonic oscillators of different frequencies; all the frequencies are represented.

Thanks.

I have a follow up question: it's easy to show that the average energy of one of these oscillators is [tex]<E>=\frac{h\nu}{e^{h\nu / kT}-1}.[/tex]

How to you go from this formula to the energy density of the electromagnetic field in equilibrium?
 
  • #4
dEdt said:
How to you go from this formula to the energy density of the electromagnetic field in equilibrium?

Imagine a cubic metal box of side length L. In this box only a discrete set of electromagnetic modes is allowed. Compute the expected energy in each mode and sum over the (infinite number of) modes. Divide by the box volume. Take ##L \to \infty## (the easy way to do this is to approximate the sum over discrete modes by an integral; this approximation becomes good in the large-L limit).
 
  • #5
dEdt said:
My question is, how can a collection of oscillators like this ever emit radiation which does not have frequency [itex]\nu[/itex] as well?
Black bodies are opaque. That means the photon does not come to your eye straight from being emitted. On the way it scatters off atoms, and each scattering results in a change of frequency. The photons and the atoms have frequent interactions, and are in thermal equilibrium with each other.
 
  • #6
The_Duck said:
Imagine a cubic metal box of side length L. In this box only a discrete set of electromagnetic modes is allowed. Compute the expected energy in each mode and sum over the (infinite number of) modes. Divide by the box volume. Take ##L \to \infty## (the easy way to do this is to approximate the sum over discrete modes by an integral; this approximation becomes good in the large-L limit).

How do you relate the expected energy in each mode to the average energy of an oscillator?
 
  • #7
Bill_K said:
Black bodies are opaque. That means the photon does not come to your eye straight from being emitted. On the way it scatters off atoms, and each scattering results in a change of frequency. The photons and the atoms have frequent interactions, and are in thermal equilibrium with each other.

It still seems like the photon's energy has to stay a multiple of ##h \nu##. If the photon's energy starts off as a multiple ##h \nu##, and if every atom's energy can only change by a multiple of ##h \nu##, then it seems like the photon's energy has to stay a multiple of ##h \nu##.
 
  • #8
dEdt said:
It still seems like the photon's energy has to stay a multiple of ##h \nu##. If the photon's energy starts off as a multiple ##h \nu##, and if every atom's energy can only change by a multiple of ##h \nu##, then it seems like the photon's energy has to stay a multiple of ##h \nu##.
No, no, what makes you think the atom's energy has to change by ##h \nu##?? We are talking about collisions and recoils, not excitation to a higher energy level. Atoms move, they carry kinetic energy! :smile: That's what thermal equilibrium is all about. A collision will transfer some of the atom's kinetic energy to or from the photon.
 
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  • #9
Bill_K said:
No, no, what makes you think the atom's energy has to change by ##h \nu##?? We are talking about collisions and recoils, not excitation to a higher energy level. Atoms move, they carry kinetic energy! :smile: That's what thermal equilibrium is all about. A head-on collision, for example, will transfer some of the atom's kinetic energy to the photon.

Right, but I'm not thinking about a real solid but rather Planck's model of a blackbody, made up of a large number of quantized oscillators. (I shouldn't have used the word atom.)
 
  • #11
dEdt said:
How do you relate the expected energy in each mode to the average energy of an oscillator?

The expected energy in a mode with frequency ##\nu## is given by your formula in post #3.
 
  • #12
dEdt said:
How do you relate the expected energy in each mode to the average energy of an oscillator?

There are more ways to do that.

The easy way is to say that the mode with the same frequency as the resonator is, albeit abstract, just another harmonic oscillator, so the average energy at a given temperature should be the same.

The hard way would be to calculate motion of the resonator under prescribed EM radiation and derive relation between average amplitudes of the EM field and that of the resonator. I think Planck did something along these lines in Part IV of his book The theory of heat radiation, Blakiston's son & Co., 1914 Philadelphia

https://archive.org/details/theheatradiation00planrich
 
  • #13
The container for the black body radiation does not have to be metal. The "standing waves" criterion comes from the requirement for thermal equilibrium. Hyperphysics and many other sites are not clear on this point. A good explanation is on then QuantumBaking channel of YouTube. There are 11 videos on black body radiation and the sixth one speaks to this point:
 
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  • #14
Renormalized said:
The container for the black body radiation does not have to be metal. The "standing waves" criterion comes from the requirement for thermal equilibrium.

True, the formal operations in the derivation of the Rayleigh-Jeans formula seem to work even if the cuboid is made of wood or has entirely fictive boundary and thus no condition is imposed on the values of the field on the walls; the assumption that the average energy due to one Fourier component is the same as average energy of ordinary harmonic oscillator - ##k_B T## - is sufficient.

However, perfectly reflecting cavity is considered in discussions of equilibrium radiation for a different, older reason: the Rayleigh-Jeans calculation addresses equilibrium radiation: existence of equilibrium requires that the system radiation + matter does not lose energy systematically through the (real of fictive) walls. Perfect conductor is able to prevent escape of EM energy, since (I believe) the Poynting vector has to have zero component normal to the walls. This way, matter can achieve thermodynamic equilibrium with radiation inside the cavity.

In a sense, perfect conductor is like adiabatic wall in thermodynamics - non-existent, but very useful in theory.

Of course, in experiments attempting to realize equilibrium radiation perfect conductors are not available, so people use next best thing - metals. Although metallic wall is not a perfect conductor, for long enough waves it is very close to being one. And even for high frequencies, it is best we can do.

By the way, this means that part of the mismatch between the Rayleigh-Jeans formula and experiment is due to the fact that we cannot really prepare equilibrium radiation for ##all## frequencies - frequencies high enough go right through the walls, since they are not made of perfect conductor.

Perhaps there are other reasons for why metallic cavity is assumed in the calculations of Rayleigh-Jeans type - if you know some, please let us know.
 
  • #15
Most experiments with black body radiation use glass or ceramic as the container. Common metals melt at typical temperatures used for black body experiments.

There is no need to prevent long radio waves and short gamma rays from penetrating the walls. All that is needed is thermal equilibrium between the radiation field and the walls. The radiation field cannot pump energy from one side of the container to the other. There must be equal amounts of left and right going waves, which is roughly equivalent to saying standing waves.
 
  • #16
Renormalized said:
Most experiments with black body radiation use glass or ceramic as the container.

I do not know how measurements of intensity of equilibrium radiation are done today exactly, but I recall the experiments of Lummer and Pringsheim used blackened metallic cavity. This works well if temperatures measured are low enough. The reason metal was used is that the metal prevents the heat radiation energy from escaping away.

Even if the radiation has temperature greater than the temperature of the metal, the metal does not have to melt, since it reflects most of the radiant energy. The little heat that does get absorbed by the metal can be removed by coolant applied from the outside so no melting occurs.

I suppose other materials can be used too inside the cavity if they help to establish and maintain state of radiation close to equilibrium. But to isolate the cavity from radiating away its energy to the outer space, metal seems best.


There is no need to prevent long radio waves and short gamma rays from penetrating the walls.

Establishment and maintaining thermal equilibrium requires that the system does not lose energy too quickly. If the walls are transparent at some frequency, I do not see how the intensity of radiation at this frequency inside the cavity could be claimed to have equilibrium value.

All that is needed is thermal equilibrium between the radiation field and the walls.

Well, if the radiation inside was at equilibrium with the walls, the walls would be penetrated by the radiation and had to have the same temperature as the radiation. Thus they would radiate away to the outer space (outside the cavity). To maintain this equilibrium, such system would have to be enclosed in a still larger reflective (metallic) cavity.

The radiation field cannot pump energy from one side of the container to the other.

Energy can flow from one side to the other, as the thermal EM field is chaotic and has fluctuations. Only on average, there should not be any transfer of energy.

There must be equal amounts of left and right going waves, which is roughly equivalent to saying standing waves.

...in equilibrium, which happens because we isolated the system well, for example by metallic cavity.
 

1. What is blackbody radiation?

Blackbody radiation is the thermal electromagnetic radiation emitted by an object that absorbs all incident electromagnetic radiation. It is also known as Planck radiation or thermal radiation.

2. How is blackbody radiation related to temperature?

The amount and wavelength of blackbody radiation emitted by an object is directly related to its temperature. As the temperature increases, the intensity of the radiation also increases and the wavelength shifts towards shorter wavelengths.

3. What is the significance of the "ν" in "Blackbody Radiation: Exploring Beyond ν"?

The "ν" represents the frequency of the radiation, which is a crucial factor in understanding blackbody radiation. In this context, "Beyond ν" refers to exploring the phenomena of blackbody radiation at frequencies beyond the visible spectrum.

4. How does blackbody radiation affect the color of objects?

The color of an object is determined by the wavelengths of light that it reflects. Blackbody radiation can affect the color of an object by changing the wavelengths of light it emits, which in turn affects the wavelengths of light that are reflected. As the temperature of an object increases, it emits shorter wavelengths of light, which can change the perceived color of the object.

5. What are some applications of blackbody radiation?

Blackbody radiation has many practical applications in fields such as astrophysics, thermodynamics, and materials science. For example, it is used in infrared thermometers to measure temperature, in solar panels to absorb sunlight and convert it into energy, and in telescopes to study the radiation emitted by astronomical objects.

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