SUMMARY
Gravity, according to General Relativity (GR), is defined as the curvature of spacetime caused by mass and energy. This concept fundamentally shifts the understanding of gravity from a force to a geometric property of spacetime. The technical definition emphasizes that massive objects like planets and stars warp the fabric of spacetime, influencing the motion of other objects. For a comprehensive understanding, refer to resources such as the "No Nonsense Introduction to General Relativity" available at Preposterous Universe.
PREREQUISITES
- Understanding of General Relativity principles
- Familiarity with spacetime concepts
- Basic knowledge of mass-energy equivalence
- Ability to interpret scientific literature on physics
NEXT STEPS
- Explore the mathematical framework of General Relativity
- Study the implications of spacetime curvature on planetary motion
- Investigate gravitational waves and their significance in GR
- Read advanced texts on the applications of GR in cosmology
USEFUL FOR
Physicists, students of theoretical physics, and anyone interested in the fundamental principles of gravity and spacetime as described by General Relativity.