SUMMARY
Atoms formed approximately 300,000 years after the Big Bang, during a process known as recombination. Initially, only hydrogen atoms were created, as the universe transitioned from a hot, ionized state to a cooler, neutral one. The photon epoch saw the annihilation of most leptons, resulting in a universe predominantly composed of ionic matter until neutral atoms could form. The first stars emerged about a billion years later, further ionizing the surrounding gas.
PREREQUISITES
- Understanding of the Big Bang Theory
- Knowledge of atomic structure and fundamental particles
- Familiarity with the concept of recombination in cosmology
- Basic grasp of the photon epoch and its implications
NEXT STEPS
- Research the process of recombination in cosmology
- Learn about the photon epoch and its significance in the universe's evolution
- Study the formation of the first stars and their impact on the universe
- Explore the timeline of the universe's history, focusing on key events post-Big Bang
USEFUL FOR
Astronomers, astrophysicists, students of cosmology, and anyone interested in the early universe and atomic formation processes.