What Happened to the Energy from Matter/Anti-Matter Annihilation?

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SUMMARY

The discussion centers on the fate of energy resulting from matter and anti-matter annihilation in the early universe. It is established that for every billion annihilations, one atom remained, leading to a significant release of energy. This energy is now identified as the cosmic microwave background (CMB), which is a remnant of the early universe's conditions. The CMB serves as a crucial piece of evidence for the Big Bang theory and the evolution of the universe.

PREREQUISITES
  • Understanding of matter and anti-matter interactions
  • Familiarity with the concept of annihilation in physics
  • Knowledge of the Big Bang theory
  • Basic grasp of cosmic microwave background radiation
NEXT STEPS
  • Research the properties and significance of cosmic microwave background radiation
  • Explore the implications of matter and anti-matter annihilation in cosmology
  • Study the Big Bang nucleosynthesis process
  • Investigate current theories regarding the early universe's conditions
USEFUL FOR

Astronomers, physicists, cosmologists, and anyone interested in the fundamental processes of the universe's formation and evolution.

phetuspolice
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I've read how in the early early universe, there were massive amounts of collisions between matter and anti-matter, about a billion of each annihilated to every atom left over.
My question is, what happened to all that energy?
 
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phetuspolice said:
I've read how in the early early universe, there were massive amounts of collisions between matter and anti-matter, about a billion of each annihilated to every atom left over.
My question is, what happened to all that energy?

Without going into a lot of detail, it is the cosmic microwave background.
 

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