SUMMARY
Dark matter is theorized to consist of exotic particles from the Big Bang, approximately 13.7 billion years ago. Its existence is inferred from gravitational effects on visible matter, as it does not emit light or heat. The discussion highlights the ongoing debate regarding dark matter's necessity in explaining astronomical observations, with some arguing for alternative theories like Modified Newtonian Dynamics (MOND). Key figures in the debate include Vera Rubin, who studied galaxy rotation curves, and Milgrom, who formulated MOND to challenge the need for dark matter.
PREREQUISITES
- Understanding of gravitational theory, particularly General Relativity.
- Familiarity with astronomical observations and their implications for dark matter.
- Knowledge of Modified Newtonian Dynamics (MOND) and its principles.
- Awareness of the historical context of Einstein's theories and their evolution.
NEXT STEPS
- Research the implications of Vera Rubin's findings on galaxy rotation curves.
- Explore the principles and predictions of Modified Newtonian Dynamics (MOND).
- Investigate recent studies on dark matter candidates and their observational evidence.
- Read Einstein's original essays on relativity and the ether for historical context.
USEFUL FOR
Astronomers, physicists, cosmologists, and anyone interested in the fundamental questions of dark matter and its role in the universe.