Triple
T12216727
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Gary W. Gibbons |
E291104
|
entity |
| Predicate | notableConcept |
P201
|
FINISHED |
| Object | Gibbons–Hawking temperature |
E57424
|
NE FINISHED |
How this triple was built (2 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: Gibbons–Hawking temperature | Statement: [Gary W. Gibbons, notableConcept, Gibbons–Hawking temperature]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Gibbons–Hawking temperature Context triple: [Gary W. Gibbons, notableConcept, Gibbons–Hawking temperature]
-
A.
Gibbons–Hawking temperature
chosen
The Gibbons–Hawking temperature is the characteristic thermal radiation temperature associated with the cosmological horizon of de Sitter space, analogous to the Hawking temperature of black holes.
-
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.
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.
-
D.
Planck temperature
The Planck temperature is the theoretical maximum meaningful temperature in physics, above which current physical theories, including quantum mechanics and general relativity, are expected to break down.
-
E.
Hartle–Hawking no-boundary proposal
The Hartle–Hawking no-boundary proposal is a quantum cosmological model suggesting that the universe is finite but without an initial temporal boundary, replacing the classical Big Bang singularity with a smooth, boundaryless beginning described by quantum gravity.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (3 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_69d6ab65923081909acfc61b7a612233 |
completed | April 8, 2026, 7:24 p.m. |
| NER | Named-entity recognition | batch_69d91c9419d48190b0037fe8edc681c4 |
completed | April 10, 2026, 3:51 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69f60aa31f548190bd4f8cfe3c55614b |
completed | May 2, 2026, 2:30 p.m. |
Created at: April 8, 2026, 9:51 p.m.