Abstract
In classical general relativity, a black hole is a solution of Einstein's equations with a region of spacetime which is causally disconnected from the asymptotic region at infinity. The boundary of such a region is called the "event horizon." The spacetime around the simplest black hole in three space dimensions is described by the Schwarzschild metric.
| Original language | English |
|---|---|
| Title of host publication | Encyclopedia of Mathematical Physics |
| Subtitle of host publication | Five-Volume Set |
| Pages | 373-382 |
| Number of pages | 10 |
| ISBN (Electronic) | 9780125126601 |
| DOIs | |
| State | Published - Jan 1 2004 |
Bibliographical note
Publisher Copyright:© 2004 Elsevier Inc. All rights reserved.
ASJC Scopus subject areas
- Medicine (miscellaneous)