SUMMARY
Gravity existed before the formation of atoms, which occurred approximately 300,000 years after the Big Bang. It acted through energy rather than matter, as described by the equation E=mc², indicating that energy can warp the fabric of space and exert gravitational effects. General Relativity is foundational to understanding the universe's motion, and while gravity's influence was negligible during the universe's hot, dense state, it became significant as the universe cooled, allowing for the formation of stars and galaxies. The discussion emphasizes the importance of quantum corrections and the role of various forces, including electromagnetic and strong nuclear forces, in the early universe.
PREREQUISITES
- Understanding of General Relativity
- Familiarity with the concept of energy-mass equivalence (E=mc²)
- Knowledge of quantum mechanics and particle physics
- Basic principles of gravitational lensing
NEXT STEPS
- Research the implications of General Relativity on cosmology
- Study gravitational lensing and its observational evidence
- Explore the role of quantum corrections in early universe physics
- Read "The First Three Minutes" for a popular-level overview of the Big Bang
USEFUL FOR
Astronomers, physicists, cosmologists, and anyone interested in the fundamental forces of the universe and the early conditions following the Big Bang.