What causes the shape of the blackbody radiation graph?

In summary: I hadn't thought of it that way. I'm not sure how that would affect the graph's continuity. In summary, the line shown is continuous because it is the sum of all the allowed emission lines.
  • #1
manenbu
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Hello, I got a question about this famous graph of the spectrum given by a heated body, showing the classical line (which goes up) and Planck's line (which gives the hill shape).

How is this line continuous? Let's say my body is a lump of hydrogen, the only points on the graph should be the balmer, lyman, paschen etc wavelength. So I understand that the hotter the body is, the emission is more energetic and has shorter wavelength. But why it shows the entire spectrum and not only the allowed emission lines?
 
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  • #2
Thermal radiation has nothing to do with atoms or molecules absorbing and emitting light due to electron state transitions. Thermal radiation originates from the vibrating charges in a body, which is why it is dependent on temperature, since temperature corresponds to the strength of the vibrations of the particles in the body.
 
  • #3
Another name for http://hyperphysics.phy-astr.gsu.edu/HBASE/bbcon.html" is "cavity radiation".
 
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  • #4
manenbu said:
How is this line continuous? Let's say my body is a lump of hydrogen, the only points on the graph should be the balmer, lyman, paschen etc wavelength.

That would be true if your body was some hydrogen atoms, somehow suspended in vacuum. Quite a different thing from what you're actually made of.

The basic answer here is the same reason why you're opaque. The brief answer is that when atoms form molecules, they gain vibrational and rotational degrees of freedom, so you have these levels as well, in-between the electronic excitation levels. Condense the matter and you have additional modes caused by the interactions between molecules. Once you get to a solid, you end up with continuous bands of absorption across most of the visual/IR range, for most substances. (But you don't have the same amount of absorption in every region, hence things have colors)

NanakiXIII said:
Thermal radiation has nothing to do with atoms or molecules absorbing and emitting light due to electron state transitions. Thermal radiation originates from the vibrating charges in a body, which is why it is dependent on temperature, since temperature corresponds to the strength of the vibrations of the particles in the body.

No, temperature corresponds to all energy states (via the statistical-thermodynamical partition function), because these are coupled. It just doesn't correspond to electronic transitions in most substances at room temperature. At higher temperatures you end up with electronic transitions. At high enough temperatures you can even have ionization/X-rays in the blackbody curve (e.g. in the thermal radiation from exploding H-bombs, and from black hole accretion discs)
 
  • #5
alxm said:
No, temperature corresponds to all energy states (via the statistical-thermodynamical partition function), because these are coupled. It just doesn't correspond to electronic transitions in most substances at room temperature. At higher temperatures you end up with electronic transitions. At high enough temperatures you can even have ionization/X-rays in the blackbody curve (e.g. in the thermal radiation from exploding H-bombs, and from black hole accretion discs)

I had never considered this, but you are right. Apologies to the original poster for giving an incomplete answer. Does the spectrum still have the same shape once you start adding these discrete lines, though?
 

1. What is a blackbody radiation graph?

A blackbody radiation graph is a visual representation of the intensity of radiation emitted by a blackbody at different wavelengths or frequencies. It follows a specific curve called the Planck curve, which describes the relationship between temperature and the intensity of emitted radiation.

2. What is the significance of a blackbody radiation graph?

A blackbody radiation graph helps us understand the relationship between temperature and radiation, which is crucial in many fields of science, including astrophysics, cosmology, and thermodynamics. It also serves as a model for understanding the behavior of other objects that emit radiation, such as stars and planets.

3. How is a blackbody radiation graph different from other types of graphs?

A blackbody radiation graph is unique because it follows a specific curve, the Planck curve, which is different from the linear or exponential curves seen in other graphs. It also represents the intensity of emitted radiation rather than the amount or concentration of a substance.

4. Can a blackbody radiation graph be used to determine the temperature of an object?

Yes, a blackbody radiation graph can be used to determine the temperature of an object by comparing its radiation curve to the Planck curve. The point where the two curves intersect corresponds to the temperature of the object.

5. How does the shape of a blackbody radiation graph change with temperature?

As the temperature of a blackbody increases, the peak of the Planck curve shifts towards shorter wavelengths, and the curve becomes broader and flatter. This means that at higher temperatures, the blackbody emits more radiation at shorter wavelengths and over a wider range of wavelengths.

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