SUMMARY
The discussion centers on the nature of the cosmic horizon and its implications for visibility of luminous objects in an expanding universe. It is established that while objects can enter the particle horizon, they do not leave it in standard matter-dominated models. However, in models dominated by a cosmological constant, such as de-Sitter expansion, no new objects enter the particle horizon, and galaxies outside the local supercluster may move beyond the event horizon, rendering them invisible. The conversation highlights the distinction between particle and event horizons, clarifying that objects within the event horizon can be perceived until their light redshifts beyond detection.
PREREQUISITES
- Understanding of cosmic horizons, specifically particle and event horizons.
- Familiarity with cosmological models, particularly de-Sitter and matter-dominated models.
- Knowledge of cosmological redshift and its implications for visibility.
- Basic grasp of general relativity and its application to cosmology.
NEXT STEPS
- Study the implications of the cosmological constant in de-Sitter models.
- Learn about the differences between particle and event horizons in cosmology.
- Explore the concept of cosmological redshift and its effects on observable light.
- Read "Understanding Einstein's Relativity" by D'Inverno for insights into cosmological models.
USEFUL FOR
Astronomers, cosmologists, physics students, and anyone interested in the fundamental concepts of the universe's expansion and the nature of cosmic horizons.