SUMMARY
The observable Cosmic Microwave Background (CMB) radiation is not limited despite the finite number of emission events that occurred during the recombination era approximately 0.38 million years after the Big Bang. The CMB photons we observe today originated from a shell with a radius of 41.6 million light-years, while the event horizon at that time had a radius of 56.7 million light-years. As the universe expands, the CMB photons continue to reach us from regions inside the event horizon, ensuring a continuous supply of observable CMB radiation. However, the rate of emissions will decline over trillions of years as the temperature of the universe decreases.
PREREQUISITES
- Understanding of the Big Bang model and its implications for cosmic evolution
- Familiarity with redshift concepts and their effects on light frequency
- Knowledge of event horizons in cosmology and their significance
- Basic grasp of blackbody radiation and photon gas behavior
NEXT STEPS
- Explore the implications of redshift on cosmic observations using "Learn about cosmological redshift and its effects on light."
- Investigate the role of event horizons in cosmology with "Study the differences between black hole event horizons and cosmological event horizons."
- Examine the properties of CMB radiation through "Research the characteristics of blackbody radiation and its relevance to the CMB."
- Utilize calculators like Jorrie’s or Gnedin’s to "Calculate the arrival times of CMB photons from various shells."
USEFUL FOR
Astronomers, cosmologists, and physics students interested in the properties of the Cosmic Microwave Background radiation and its implications for the understanding of the universe's evolution.