|
Definition |
| Black hole |
A region in space where gravity is so strong that nothing, not even light, can escape from it. |
| Event horizon |
The boundary surrounding a black hole beyond which nothing can escape its gravitational pull. |
| Singularity |
A point within a black hole where gravity becomes infinitely strong and spacetime curvature becomes infinite. |
| Gravitational collapse |
The process by which massive stars collapse under their own gravity to form black holes. |
| Schwarzschild radius |
The radius of the event horizon of a non-rotating black hole. |
| Hawking radiation |
Radiation emitted by black holes due to quantum effects near the event horizon, predicted by physicist Stephen Hawking. |
| Accretion disk |
A rotating disk of matter that forms around a black hole as it pulls in surrounding gas and dust. |
| Supermassive black hole |
A black hole with a mass millions or billions of times greater than that of the Sun, found at the center of most galaxies. |
| Quasar |
A luminous object powered by an active galactic nucleus, thought to be fueled by the accretion of material onto a supermassive black hole. |
| Neutron star |
A highly compact star composed primarily of neutrons, formed from the collapsed core of a massive star. |
| White dwarf |
A small, dense star composed of electron-degenerate matter, formed from the remnants of a low to medium mass star. |
| Gravitational waves |
Ripples in spacetime caused by the acceleration of massive objects, such as black holes or neutron stars. |
| Black Hole Information Paradox |
The theoretical problem concerning the loss of information about the initial state of matter swallowed by a black hole, which contradicts the principles of quantum mechanics. |