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Black Holes
Regions in space where the gravitational pull is so strong that nothing, not even light, can escape from them.
Event Horizon
The boundary surrounding a black hole beyond which no information or matter can escape.
Escape Velocity
The minimum speed needed for an object to break free from the gravitational attraction of a celestial body.
Singularity
A point in a black hole where gravitational forces compress matter to infinitely small volume, and spacetime curvature becomes infinite.
Hawking Radiation
Thermal radiation predicted to be emitted by black holes due to quantum effects near the event horizon.
Quantum Theory of Gravity
A theoretical framework that seeks to describe gravity according to the principles of quantum mechanics.
Quantum Entanglement
A phenomenon where pairs or groups of particles become interconnected in such a way that the quantum state of one particle cannot be described independently of the others.
Black Hole Information Paradox
The dilemma regarding the fate of information that falls into a black hole and whether it is destroyed or preserved.
Emergent Spacetime
The hypothesis that space and time are not fundamental entities but emerge from more basic underlying structures or interactions.
General Relativity
Einstein's theory of gravitation that describes gravity as the curvature of spacetime caused by mass.
Quantum Mechanics
The branch of physics dealing with the behavior of matter and light on very small scales, such as atoms and subatomic particles.
Gravitational Pull
The force exerted by a mass, attracting other masses toward its center.