Relativity and gravitational theory Black holes Problem
Black hole information paradox
Problem
Suppose a black hole forms from matter in a pure quantum state and then evaporates completely by Hawking radiation. In Hawking's semiclassical computation the radiation is exactly thermal, so the final state is mixed. A map from pure states to mixed states cannot be a unitary evolution, as quantum mechanics requires. The problem is to decide whether the evaporation of a black hole is unitary. If it is, the problem is to explain how the information about the initial state is carried out by the radiation.
Remarks
Hawking stated the paradox in 1976 and argued at first that unitarity fails in gravitational collapse. Page observed in 1993 that unitarity has a consequence for the entanglement entropy of the emitted radiation. It must rise and then fall back to zero, following what is now called the Page curve. The turning point comes roughly when the black hole has lost half of its Bekenstein–Hawking entropy. The AdS/CFT correspondence describes some black holes by an ordinary unitary quantum theory, and this has led many physicists to expect unitarity. Since 2019, semiclassical computations of entropy that include so-called islands have reproduced the Page curve in several models. There is no consensus on the mechanism, and the problem remains open as a question of physics.
Reading path
To understand this page from the ground up, read these 18 pages in order. The foundations come first.
Show the path as a graph
- no evidence level
- Cauchy surface concept
- Congruence of geodesics concept
- Einstein field equations concept
- Energy conditions concept
- Event horizon concept
- Geodesic concept
- Killing horizon concept
- Killing vector field concept
- Lorentzian manifold concept
- Ricci curvature concept
- Wave equation concept
- Penrose–Hawking singularity theorems statement
- Raychaudhuri equation statement
- Hawking area theorem statement
- Laws of black hole mechanics statement
- Hawking radiation statement
- Bekenstein–Hawking entropy statement
- Black hole information paradox problem
Further reading
About this page
| Tag | 6ETFPK0E2G |
|---|---|
| URI | m2://6ETFPK0E2G |
| Kind | problem |
| Writing | W0 stub |
| MSC | 83C47, 83C57, 81P45 |
| Status | This copy of the site has no build data. Run m2 status 6ETFPK0E2G. |
| About | Black hole, Hawking radiation |
| Uses | Hawking radiation, Bekenstein–Hawking entropy |
| Changed | 3 November 2026 |
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