SUMMARY
The discussion clarifies that the "dark era" of the universe refers to a period before the formation of stars, characterized by the absence of new photon production in the visible spectrum. While no new light was generated, Cosmic Microwave Background (CMB) radiation existed, consisting of photons that were emitted during atomic formation. These CMB photons, primarily in the microwave range, were not absorbed by hydrogen atoms due to their energy being lower than the ionization threshold of hydrogen (5.87433 eV). The dark era concludes with the formation of the first stars, marking the transition to a light-filled universe.
PREREQUISITES
- Understanding of Cosmic Microwave Background (CMB) radiation
- Knowledge of atomic formation and hydrogen ionization energy
- Familiarity with electromagnetic spectrum and photon behavior
- Basic concepts of cosmology and the timeline of the universe
NEXT STEPS
- Research the properties and significance of Cosmic Microwave Background (CMB) radiation
- Study the process of atomic formation and its role in the early universe
- Explore the concept of hydrogen ionization and its implications in astrophysics
- Investigate the timeline of star formation and its impact on cosmic evolution
USEFUL FOR
Astronomers, astrophysicists, and students of cosmology who seek to understand the early universe and the significance of the dark era in cosmic history.