Why is blackbody radiation continuous?

In summary: At room temperature, collisional excitations are typically dominant. But if that is the case, what about blackbodies permits continuous spectra at all wavelengths? Why do certain materials (e.g. carbon nanotube structures) approximate well this behaviour despite being finite in size and available energy levels? Why do we not discuss/observe blackbody emissions as having discrete energies?It's worth noting that blackbody radiation isn't the only type of radiation emitted by a hot object. There's also thermal radiation, which is just the energy that's radiated away without being absorbed or reflected.
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TheCanadian
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Plasmas can emit radiation based on the acceleration of charged particles (which we generally consider as continuous), but for un-ionized matter compounds, transitions are quantized and photons have particular energies. At room temperature, collisional excitations are typically dominant. But if that is the case, what about blackbodies permits continuous spectra at all wavelengths? Why do certain materials (e.g. carbon nanotube structures) approximate well this behaviour despite being finite in size and available energy levels? Why do we not discuss/observe blackbody emissions as having discrete energies?
 
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First, a blackbody is an idealisation. Real objects only approximate a blackbody spectrum; see for instance the spectrum of the sun: https://i.stack.imgur.com/tc0Mq.png

Second, only isolated systems can be seen has having well-defined energy levels. For a gas, you have to consider in particular Doppler broadening and collision broadening. In solids, the constituent atoms loose their individual character and energy levels become energy bands.
 
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TheCanadian said:
Plasmas can emit radiation based on the acceleration of charged particles (which we generally consider as continuous), but for un-ionized matter compounds, transitions are quantized and photons have particular energies. At room temperature, collisional excitations are typically dominant. But if that is the case, what about blackbodies permits continuous spectra at all wavelengths? Why do certain materials (e.g. carbon nanotube structures) approximate well this behaviour despite being finite in size and available energy levels? Why do we not discuss/observe blackbody emissions as having discrete energies?

I have a slightly different answer than Dr. Claude: When an electromagnetic field within a cavity is at thermal equilibrium (at some temperature T), the spectrum is named 'blackbody radiation'. The spectrum is continuous because in the thermodynamic limit, the cavity dimensions are much larger than wavelengths. Micro- and nano-cavities do not exhibit the usual blackbody spectrum:

https://www.osapublishing.org/abstract.cfm?uri=QELS-1995-QTuG19
https://www.ncbi.nlm.nih.gov/pubmed/17358533
https://www.osapublishing.org/abstract.cfm?uri=QELS-2003-QWA25
 
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1. Why is blackbody radiation continuous?

The concept of blackbody radiation is based on the idea that all objects emit electromagnetic radiation, regardless of their temperature. This radiation is continuous because it is produced by the random movement of charged particles, such as electrons, within the object. As these particles move, they create changes in the electric and magnetic fields around them, resulting in the emission of electromagnetic radiation.

2. What determines the wavelength of blackbody radiation?

The wavelength of blackbody radiation is determined by the temperature of the object emitting the radiation. This is known as Wien's displacement law, which states that the peak wavelength of the radiation increases as the temperature of the object increases. Therefore, the hotter the object, the shorter the wavelength of its emitted radiation.

3. How is blackbody radiation related to the color of an object?

The color of an object is determined by the wavelengths of visible light that it reflects or emits. A blackbody, by definition, absorbs all incoming radiation and therefore appears black. However, as the temperature of the blackbody increases, it will emit radiation at all wavelengths, including visible light. The color of the object will appear to change as the temperature increases, with lower temperatures appearing red and higher temperatures appearing blue or white.

4. Can blackbody radiation be observed in real-life objects?

Yes, blackbody radiation can be observed in real-life objects. While a perfect blackbody does not exist, many objects come close to exhibiting blackbody radiation, such as stars and planets. Scientists also use controlled experiments with objects, such as a cavity with a small hole, to observe blackbody radiation and study its properties.

5. What is the importance of understanding blackbody radiation?

Understanding blackbody radiation is crucial for various fields of science, including astrophysics, energy production, and climate science. It allows scientists to predict the behavior of objects based on their temperature and wavelength of radiation. Additionally, the study of blackbody radiation has led to the development of important theories, such as Planck's law and the Stefan-Boltzmann law, which have advanced our understanding of the universe and the laws of thermodynamics.

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