SUMMARY
Physicists utilize the Friedmann equation to measure the time before the Cosmic Microwave Background (CMB) and the universe's temperature at that epoch. The CMB is established to have occurred 379,000 years after the Big Bang (BB). The temperature T(t) is inversely proportional to the scale factor a(t), which is derived from the Friedmann equation, an ordinary differential equation that describes the universe's expansion under the assumption of uniform energy distribution. This equation is a simplified version of Einstein's General Relativity equations.
PREREQUISITES
- Understanding of the Friedmann equation
- Knowledge of General Relativity principles
- Familiarity with ordinary differential equations
- Basic concepts of cosmology and the Big Bang theory
NEXT STEPS
- Study the derivation and applications of the Friedmann equation
- Learn about the implications of the Cosmic Microwave Background in cosmology
- Explore the relationship between temperature and scale factor in expanding universes
- Investigate the role of density parameters in cosmological models
USEFUL FOR
Astronomers, physicists, cosmologists, and students interested in the early universe and the mathematical modeling of cosmic expansion.