SUMMARY
The universe is definitively 13.8 billion years old, measured from the Big Bang, which is not an initial singularity but a hot, dense state marking the beginning of time as we understand it. Concepts such as gravitational time dilation do not apply in this cosmological context, as they rely on stationary spacetimes, which the universe is not. The energy density at the time of the Big Bang was finite, and while it was much larger than today, it does not imply infinite age or energy. The Cosmic Microwave Background (CMB) radiation provides evidence for this finite age, occurring approximately 380,000 years post-Big Bang.
PREREQUISITES
- Understanding of the Big Bang theory and its implications
- Familiarity with the concept of Cosmic Microwave Background (CMB) radiation
- Knowledge of gravitational time dilation and its limitations in cosmology
- Basic grasp of energy density and its relevance in cosmological contexts
NEXT STEPS
- Research the implications of the Cosmic Microwave Background (CMB) in cosmology
- Study the principles of gravitational time dilation in general relativity
- Explore the concept of energy density in the early universe
- Investigate the differences between singularities and the Big Bang in modern cosmology
USEFUL FOR
Cosmologists, astrophysicists, students of physics, and anyone interested in understanding the age and evolution of the universe.