How do we measure energy density of radiation?

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SUMMARY

The energy density of radiation is primarily attributed to the Cosmic Microwave Background (CMB), which has been measured directly and accounts for approximately 10-4 of the total energy density in the universe. The energy densities of matter and vacuum are approximately 0.3 and 0.7, respectively, with the latter associated with dark energy and measured through the universe's expansion rate. Contributions from events like supernovae are negligible in comparison to the CMB's dominance in radiation energy density.

PREREQUISITES
  • Understanding of Cosmic Microwave Background (CMB) radiation
  • Familiarity with energy density concepts in cosmology
  • Knowledge of gravitational lensing and its measurement techniques
  • Basic principles of dark energy and its implications on cosmic expansion
NEXT STEPS
  • Research the methods used to measure Cosmic Microwave Background (CMB) radiation
  • Explore the implications of dark energy on the universe's expansion rate
  • Study gravitational lensing techniques and their applications in cosmology
  • Investigate the role of supernovae in cosmic energy contributions
USEFUL FOR

Astronomers, cosmologists, and physics students interested in understanding the energy dynamics of the universe and the significance of the Cosmic Microwave Background in cosmological measurements.

binbagsss
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I have that the energy density of matter approx 0.3 , so this is measured by galaxy motion / gravitational lensing etc, that's fine.

I have that the energy density due to the vacuum is 0.7, so this is measured by the expansion rate- the common suspect being dark energy.

I have radiation contribution approx 10^{-4}. How is this measured? Or is this theoretical?

Thanks
 
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The radiation density is the energy density of the CMB, and has been measured directly.
 
Chalnoth said:
The radiation density is the energy density of the CMB, and has been measured directly.

nothing else contributes? like when a star explodes, the EM radiation given off then e.g?
 
binbagsss said:
nothing else contributes? like when a star explodes, the EM radiation given off then e.g?
Not to any significant degree. The CMB comprises nearly all of the radiation ever emitted, by energy density.
 
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