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A typical black hole is always specified by
a (curvature) singularity
either a (curvature) singularity or a horizon
Black holes are regions of spacetime from which nothing, not even light, can escape. A typical black hole is the result of the gravitational force becoming so strong that one would have to travel faster than light to escape its pull. Such black holes contain a spacetime singularity at their centre.
By: Parvesh Mehta ProfileResourcesReport error
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