SUMMARY
The cosmological redshift is primarily caused by the metric expansion of space, which stretches photons as they travel through the universe. This phenomenon results in a shift of light towards longer wavelengths, typically observed as redshift in distant galaxies. Compton scattering with free electrons in stellar atmospheres does not contribute to cosmological redshift, as it cannot shift emission lines to different wavelengths. Instead, the redshift is accurately measured through specific emission lines unique to each atom, which remain consistent despite the expansion of space.
PREREQUISITES
- Understanding of cosmological redshift and its implications in astrophysics
- Familiarity with General Relativity and its effects on energy conservation
- Knowledge of emission and absorption lines in atomic physics
- Basic concepts of the Doppler effect in relation to light
NEXT STEPS
- Study the metric expansion of space and its role in cosmology
- Learn about the Doppler effect and its application to light from moving sources
- Explore the significance of emission lines in spectroscopy for measuring redshift
- Investigate the implications of General Relativity on energy conservation in cosmological contexts
USEFUL FOR
Astronomers, astrophysicists, and students of cosmology seeking to deepen their understanding of redshift phenomena and the underlying principles of light behavior in an expanding universe.