SUMMARY
The initial temperature of the Big Bang cannot be defined as a singular value due to the nature of the Big Bang being a process rather than an event. The temperature right after reheating, caused by the decay of the inflaton, is the closest approximation, but the exact energy density remains unknown. The temperature of the cosmic microwave background (CMB) radiation is approximately 3K, while the temperature at the earliest moments is thought to be around one-third of the Planck temperature. Understanding these concepts requires recognizing that properties like time and temperature are undefined at t=0.
PREREQUISITES
- Understanding of cosmic microwave background (CMB) radiation
- Familiarity with inflation theory in cosmology
- Knowledge of Planck temperature and its significance
- Basic grasp of redshift and its relation to temperature
NEXT STEPS
- Research the implications of inflation theory on early universe temperatures
- Explore the concept of Planck temperature and its relevance in cosmology
- Study the relationship between redshift and temperature in the context of the CMB
- Investigate alternative theories to inflation and their predictions for initial conditions
USEFUL FOR
Astronomers, cosmologists, physics students, and anyone interested in the fundamental properties of the universe and the Big Bang theory.