Electromagnetic Radiation temperature

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SUMMARY

The discussion centers on the relationship between electromagnetic radiation and temperature, specifically how the universe's temperature of 2.7 Kelvin is derived from cosmic microwave background radiation. It emphasizes that a blackbody in thermal equilibrium with radiation can be assigned a temperature equivalent to that radiation. The conversation also highlights the importance of thermal distribution among molecules for defining temperature and how this concept applies to photons, which can be assigned a temperature if their spectral distribution resembles that of a blackbody spectrum.

PREREQUISITES
  • Understanding of blackbody radiation and its significance in thermodynamics
  • Familiarity with the concept of thermal equilibrium
  • Knowledge of statistical mechanics and kinetic energy distribution
  • Basic principles of electromagnetic radiation and photon behavior
NEXT STEPS
  • Research the properties of blackbody radiation and Planck's Law
  • Explore the implications of Hawking radiation on cosmic temperature
  • Study the statistical mechanics of thermal distributions and their applications
  • Investigate the relationship between photon spectra and temperature in astrophysics
USEFUL FOR

Astrophysicists, thermodynamic researchers, and students of physics interested in the interplay between electromagnetic radiation and temperature in cosmic contexts.

Df241
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Is there a meaningful way to convert the energy of an electromagnetic wave to a temperature? I mean this more along the lines of how the universe has a temperature of 2.7 kelvin due to electromagnetic radiation. I'm honestly just curious to determine the temperature of the universe after nearly all normal matter has gone into a black hole and radiated as Hawking radiation.
 
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If a blackbody at a given temperature and immersed in the radiation would be in equilibrium, neither heating up nor cooling off, then we can meaningfully say that the temperature of the blackbody is the tenperature of the radiation. That's how we arrive at 2.7 degrees as the temperature of the cosmic microwave background.

If the blackbody were to cool off by radiating away more energy than it absorbs, then we would say that the temperature of the blackbody is greater than that of the radiation, and vice versa.
 
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To expand on what Nugatory said, temperature is statistical. For example if I have one molecule it doesn't have a temperature, it has a kinetic energy. When we have lots of molecules we only say they have a temperature if their kinetic energy is distributed something similar to the distribution they would have at thermal equilibrium. They don't have to be at thermal equilibrium, but the distribution has to be thermal or close to thermal for us to label it with a temperature. The thermal distribution arises from how energy is shared among the molecules by random processes, and a thermal distribution allows us to reason by thermodynamics how that energy will be shared with another body in thermal contact again by random statistical processes. If the distribution isn't thermal, say all the molecules were shot out of an accelerator with a narrow distribution of energies, then if we try and associate the kinetic energy with a temperature and use thermodynamics to say what will happen when the molecules hit a target or the wall we will be wrong. The laws of thermodynamics and thermodynamic calculations are based on the idea that the kinetic energy is being randomly shared among the degrees of freedom.

Well light is the same. A stream of photons is said to have a temperature if it has a distribution (and with light that means spectrum or more precisely a distribution in spectral density) that is similar to the spectrum that would arise from random thermal processes, i.e. a blackbody spectrum. If it has that distribution we can use temperature and thermodynamic reasoning to say what will happen if that light impinges on an object i.e. we can say the light spectrum has a temperature. If it doesn't have that spectrum and we try to reason thermodynamically we will be wrong.
 
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