SUMMARY
Energy cannot be created or destroyed, only converted from one form to another, as established by the law of conservation of energy. This principle is encapsulated in Einstein's equation E=mc², where E represents energy, m represents mass, and c denotes the speed of light (approximately 3×108 m/s). While mass can be lost in nuclear processes, such as during nuclear fission, the overall conservation of energy remains unviolated. The discussion also touches on the concept of supersymmetry, which suggests that conservation laws must hold for all observers.
PREREQUISITES
- Understanding of Einstein's equation E=mc²
- Basic knowledge of nuclear fission processes
- Familiarity with the law of conservation of energy
- Introductory concepts of supersymmetry in physics
NEXT STEPS
- Research the implications of E=mc² in modern physics
- Study the principles of nuclear fission and its energy release
- Explore the concept of supersymmetry and its relevance to conservation laws
- Investigate empirical evidence supporting the law of conservation of energy
USEFUL FOR
Students of physics, educators, and anyone interested in understanding fundamental principles of energy and matter conservation.