SUMMARY
The mass of a black hole is fundamentally a property of spacetime geometry rather than a composition of particles such as neutrons, protons, or electrons. When a star collapses into a black hole, the matter that constituted the star is believed to be destroyed at the singularity, where classical physics breaks down. The concept of mass in this context differs from mass derived from particle interactions with the Higgs field, emphasizing the need to distinguish between these definitions. Current understanding suggests that the mass of a black hole does not consist of traditional matter but is instead a manifestation of the spacetime curvature resulting from the energy that formed it.
PREREQUISITES
- General Relativity (GR) principles
- Understanding of spacetime geometry
- Basic particle physics, particularly the Higgs field
- Familiarity with singularities and their implications in physics
NEXT STEPS
- Explore the implications of singularities in General Relativity
- Research quantum gravity theories and their relation to black holes
- Study the Schwarzschild metric and its significance in black hole physics
- Investigate the role of the Higgs field in particle mass generation
USEFUL FOR
Physicists, astrophysicists, and students of theoretical physics interested in black hole mechanics, spacetime properties, and the intersection of quantum mechanics and general relativity.