click below
click below
Normal Size Small Size show me how
Black Holes
Black Hole notes
| Question | Answer |
|---|---|
| Black Hole | Astronomical entity with gravity so strong that light cannot escape. |
| Gravitational Singularity | Point at the center of a black hole where density and spacetime curvature become infinite. |
| TOV Limit | Maximum mass limit for a stable neutron star beyond which it collapses into a black hole. |
| The boundary surrounding a black hole marking the point of no return where escape velocity equals light speed. | |
| Schwarzschild Radius | Radius defining the event horizon of a non-rotating black hole, calculated as r = 2GM/c². |
| Spaghettification | Stretching of objects due to extreme tidal gravitational forces near a black hole's event horizon. |
| No-Hair Theorem | Principle stating that black holes are completely characterized by only three parameters: mass, charge, and angular momentum. |
| Kerr Metric | Metric describing rotating black holes possessing mass and angular momentum. |
| Ergosphere | Pumpkin-shaped region outside a rotating Kerr black hole's event horizon where frame-dragging forces spacetime to rotate. |
| Penrose Process | Mechanism by which energy can be extracted from the ergosphere of a rotating black hole. |
| Super-radiance | Process where waves scattering off a rotating black hole's ergosphere gain energy, potentially creating a "black hole bomb". |
| Hawking Radiation | Thermal blackbody radiation emitted near the event horizon due to quantum pair creation, causing black holes to evaporate. |
| Black Hole Information Paradox | Paradox regarding whether physical information is lost when matter falls into a black hole and evaporates. |
| Holographic Principle | Theory suggesting that all volume information inside a black hole is encoded on its boundary event horizon. |
| Supermassive Black Hole (SMBH) | Black holes millions to billions of solar masses found at the centers of galaxies like the Milky Way. |
| Sagittarius A* | Supermassive black hole located at the center of the Milky Way galaxy. |
| Event Horizon Telescope (EHT) | Global radio telescope array using VLBI to capture direct images of black hole shadows (M87* and Sgr A*). |
| Katie Bouman | Computer scientist who led the development of the CHIRP algorithm used to reconstruct EHT images. |
| LIGO | Observatory that made the first direct detection of gravitational waves from binary black hole mergers. |
| Andrea Ghez | Astronomer awarded the 2020 Nobel Prize in Physics for discovering the supermassive compact object Sagittarius A*. |