SUMMARY
The first atoms, primarily Hydrogen and Helium, were created several hundred thousand years after the Big Bang, during a period when the Universe was a hot plasma. According to Dalton's atomic theory, atoms cannot be created or destroyed, but matter can emerge from pure radiation if conservation laws are satisfied. The processes of nuclear fission and fusion also lead to the creation of new atoms from existing ones. For a deeper understanding of nucleosynthesis, Weinberg's 'First Three Minutes' provides a comprehensive overview of the early Universe's matter creation.
PREREQUISITES
- Understanding of Dalton's atomic theory
- Familiarity with nuclear fission and fusion processes
- Knowledge of conservation laws in physics
- Basic concepts of nucleosynthesis
NEXT STEPS
- Read Weinberg's 'First Three Minutes' for insights on early Universe nucleosynthesis
- Explore the concept of pair production in quantum physics
- Investigate the conditions of the Universe during the Big Bang
- Study the processes of nuclear fusion in stars
USEFUL FOR
Physicists, cosmologists, and students interested in the origins of matter and the early Universe's conditions.