black hole complementarity
E725131
Black hole complementarity is a theoretical principle in quantum gravity proposing that information falling into a black hole is both reflected at the event horizon and passes through it, with no single observer able to witness any violation of quantum mechanics or general relativity.
All labels observed (1)
| Label | Occurrences |
|---|---|
| black hole complementarity canonical | 2 |
How this entity was disambiguated
This entity first appeared as the object of triple T8325776 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: black hole complementarity Context triple: [Leonard Susskind, knownFor, black hole complementarity]
-
A.
black hole no-hair theorem
The black hole no-hair theorem is a principle in general relativity stating that stationary black holes are completely characterized by only a few macroscopic parameters—mass, electric charge, and angular momentum—regardless of the details of the matter that formed them.
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B.
Bekenstein–Hawking entropy
Bekenstein–Hawking entropy is the thermodynamic entropy associated with a black hole, proportional to the area of its event horizon and fundamental in linking gravity, quantum theory, and thermodynamics.
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C.
holographic principle
The holographic principle is a theoretical physics concept proposing that all the information contained within a volume of space can be represented as encoded data on its boundary, much like a hologram.
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D.
cosmic censorship conjecture
The cosmic censorship conjecture is a hypothesis in general relativity proposing that singularities arising from gravitational collapse are always hidden within event horizons, preventing "naked" singularities from being observed.
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E.
Hawking radiation
Hawking radiation is the theoretical blackbody radiation predicted to be emitted by black holes due to quantum effects near the event horizon, causing them to lose mass and eventually evaporate.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: black hole complementarity Target entity description: Black hole complementarity is a theoretical principle in quantum gravity proposing that information falling into a black hole is both reflected at the event horizon and passes through it, with no single observer able to witness any violation of quantum mechanics or general relativity.
-
A.
black hole no-hair theorem
The black hole no-hair theorem is a principle in general relativity stating that stationary black holes are completely characterized by only a few macroscopic parameters—mass, electric charge, and angular momentum—regardless of the details of the matter that formed them.
-
B.
Bekenstein–Hawking entropy
Bekenstein–Hawking entropy is the thermodynamic entropy associated with a black hole, proportional to the area of its event horizon and fundamental in linking gravity, quantum theory, and thermodynamics.
-
C.
holographic principle
The holographic principle is a theoretical physics concept proposing that all the information contained within a volume of space can be represented as encoded data on its boundary, much like a hologram.
-
D.
cosmic censorship conjecture
The cosmic censorship conjecture is a hypothesis in general relativity proposing that singularities arising from gravitational collapse are always hidden within event horizons, preventing "naked" singularities from being observed.
-
E.
Hawking radiation
Hawking radiation is the theoretical blackbody radiation predicted to be emitted by black holes due to quantum effects near the event horizon, causing them to lose mass and eventually evaporate.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
proposal in quantum gravity
ⓘ
theoretical principle ⓘ |
| addresses | black hole information paradox ⓘ |
| aimsToPreserve |
equivalence principle at the horizon
ⓘ
unitarity ⓘ |
| associatedWith |
Gerard ’t Hooft
ⓘ
John Preskill ⓘ Larus Thorlacius ⓘ Leonard Susskind ⓘ |
| assumes |
measurements are limited by causal structure around the horizon
ⓘ
no observer can both fall into and remain outside the same black hole ⓘ |
| challengedBy |
AMPS firewall argument
ⓘ
black hole firewall paradox ⓘ |
| compatibleWith |
equivalence principle for infalling observers
ⓘ
unitary evolution of quantum states ⓘ |
| concerns |
consistency of quantum field theory in curved spacetime
ⓘ
information flow in black hole evaporation ⓘ |
| contrastsWith | Hawking’s original information loss proposal ⓘ |
| describedAs | complementarity between infalling and external observers ⓘ |
| field |
black hole physics
ⓘ
quantum gravity ⓘ theoretical physics ⓘ |
| implies |
apparent information cloning is not operationally observable
ⓘ
description of physics depends on observer’s worldline ⓘ no observer can access both interior and exterior information copies ⓘ |
| influenced |
AdS/CFT correspondence interpretations
ⓘ
development of the holographic principle ⓘ |
| motivatedBy |
Hawking’s argument for information loss
ⓘ
conflict between quantum mechanics and semiclassical gravity ⓘ |
| proposes |
different observers have complementary descriptions of the same physical process
ⓘ
information falling into a black hole also passes through the event horizon ⓘ information falling into a black hole is effectively reflected at the event horizon ⓘ information is not lost in black holes ⓘ no single observer can see a violation of general relativity ⓘ no single observer can see a violation of quantum mechanics ⓘ |
| relatesTo |
Hawking radiation
ⓘ
black hole entropy ⓘ equivalence principle ⓘ event horizon ⓘ holographic principle ⓘ no-cloning theorem ⓘ stretched horizon ⓘ unitarity of quantum mechanics ⓘ |
| status |
controversial
ⓘ
hypothetical ⓘ |
| timePeriod | early 1990s ⓘ |
| usesConcept |
observer-dependent horizons
ⓘ
stretched horizon as a physical membrane ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: black hole complementarity Description of subject: Black hole complementarity is a theoretical principle in quantum gravity proposing that information falling into a black hole is both reflected at the event horizon and passes through it, with no single observer able to witness any violation of quantum mechanics or general relativity.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.