SUMMARY
The Friedmann equations are invalid at the moment of the Big Bang, specifically at time t=0, due to the presence of a singularity. Solutions to the Friedmann equations do not include the Big Bang as a point in time and instead begin just after this moment. Current observations suggest that these equations are reliable after a few minutes post-Big Bang, particularly supported by Big Bang Nucleosynthesis data. However, their applicability before this time remains uncertain and requires further exploration.
PREREQUISITES
- Understanding of Friedmann equations in cosmology
- Knowledge of singularities in general relativity
- Familiarity with Big Bang Nucleosynthesis
- Basic concepts of time in cosmological models
NEXT STEPS
- Research the implications of singularities in general relativity
- Explore alternative cosmological models that address pre-Big Bang conditions
- Study the role of Big Bang Nucleosynthesis in validating cosmological theories
- Investigate current advancements in observational cosmology
USEFUL FOR
Astronomers, physicists, and cosmologists interested in the foundations of the universe and the validity of cosmological equations at critical moments in time.