Triple
T8325776
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Leonard Susskind |
E194947
|
entity |
| Predicate | knownFor |
P22
|
FINISHED |
| Object |
black hole complementarity
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.
|
E725131
|
NE FINISHED |
How this triple was built (4 steps)
Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.
NER
Named-entity recognition
gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: black hole complementarity | Statement: [Leonard Susskind, knownFor, black hole complementarity]
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.
-
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
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg
Description generation
gpt-5.1
Instruction
Generate a one-sentence description of the target entity. You are given a context triple in the form (subject, predicate, object), where the object is the target entity. # Instructions Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. Avoid repeating the information from the triple, unless really essential. # Response Format Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: black hole complementarity Triple: [Leonard Susskind, knownFor, black hole complementarity]
Generated 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.
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
Provenance (5 batches)
The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.
| Step | Stage | Batch ID | Status | When |
|---|---|---|---|---|
| creating | Elicitation | batch_69ca82e7a8a88190a32bb5cc0feb012d |
completed | March 30, 2026, 2:04 p.m. |
| NER | Named-entity recognition | batch_69cb7f7fba688190b696593dfb2cde5d |
completed | March 31, 2026, 8:02 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69cd95b22afc81909c867d83a1744139 |
completed | April 1, 2026, 10:01 p.m. |
| NEDg | Description generation | batch_69cdab60ec308190a9001f9235e556b4 |
completed | April 1, 2026, 11:33 p.m. |
| NED2 | Entity disambiguation (via description) | batch_69cdb2e3457c8190a2d0cb6eeb81c9ef |
completed | April 2, 2026, 12:05 a.m. |
Created at: March 30, 2026, 5:56 p.m.