SUMMARY
The early universe was predominantly opaque due to photon scattering off free electrons, a process known as Thomson scattering. Scattering off protons is significantly less impactful because the Thomson scattering cross section is inversely proportional to the square of the mass, resulting in a suppression factor of approximately one million for protons compared to electrons. This phenomenon is rooted in classical physics, where lighter particles like electrons experience greater acceleration from electromagnetic radiation, leading to more effective scattering. The discussion also touches on the implications of this effect in stellar environments.
PREREQUISITES
- Understanding of Thomson scattering and its role in astrophysics
- Familiarity with the concepts of mass and acceleration in classical mechanics
- Basic knowledge of Compton scattering and Feynman diagrams
- Awareness of the early universe's conditions and photon interactions
NEXT STEPS
- Research the mathematical derivation of the Thomson scattering cross section
- Explore the differences between Thomson scattering and Compton scattering
- Study the implications of particle mass on scattering probabilities
- Investigate the role of scattering in stellar evolution and opacity
USEFUL FOR
Astronomers, physicists, and students of cosmology interested in the interactions of photons with matter in the early universe and stellar environments.