24: Black Holes and Curved Spacetime Flashcards
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
accretion disk
a region in spacetime where gravity is so strong that nothing—not even light—can escape
black hole
concept that a gravitational force and a suitable acceleration are indistinguishable within a sufficiently local environment - free-fall and zero gravity are the same
equivalence principle
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
event horizon
Einstein’s theory relating gravity and the structure (geometry) of space and time
general theory of relativity
an increase in wavelength of an electromagnetic wave (light) when propagating from or near a massive object
gravitational redshift
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
gravitational wave
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
singularity
system of one time and three space coordinates, with respect to which the time and place of an event can be specified
spacetime
term for the way an object is stretched in the direction of a black hole
spaghettification