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24.9: Key Terms

Last updated

Jul 28, 2023
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- 24.8: Gravitational Wave Astronomy
- 24.10: Summary

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accretion disk: the disk of gas and dust found orbiting newborn stars, as well as compact stellar remnants such as white dwarfs, neutron stars, and black holes when they are in binary systems and are sufficiently close to their binary companions to draw off material

black hole: a region in spacetime where gravity is so strong that nothing—not even light—can escape

equivalence principle: concept that a gravitational force and a suitable acceleration are indistinguishable within a sufficiently local environment

event horizon: a boundary in spacetime such that events inside the boundary can have no effect on the world outside it—that is, the boundary of the region around a black hole where the curvature of spacetime no longer provides any way out

general theory of relativity: Einstein’s theory relating gravity and the structure (geometry) of space and time

gravitational redshift: an increase in wavelength of an electromagnetic wave (light) when propagating from or near a massive object

gravitational wave: a disturbance in the curvature of spacetime caused by changes in how matter is distributed; gravitational waves propagate at (or near) the speed of light.

singularity: the point of zero volume and infinite density to which any object that becomes a black hole must collapse, according to the theory of general relativity

spacetime: system of one time and three space coordinates, with respect to which the time and place of an event can be specified

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