Triple
T10147864
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | The four laws of black hole mechanics |
E231749
|
entity |
| Predicate | foundationFor |
P1450
|
FINISHED |
| Object | Bekenstein–Hawking entropy |
E4708
|
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: Bekenstein–Hawking entropy | Statement: [The four laws of black hole mechanics, foundationFor, Bekenstein–Hawking entropy]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Bekenstein–Hawking entropy Context triple: [The four laws of black hole mechanics, foundationFor, Bekenstein–Hawking entropy]
-
A.
Bekenstein–Hawking entropy
chosen
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.
-
B.
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.
-
C.
Bekenstein bound
The Bekenstein bound is a theoretical limit in physics on the maximum amount of information or entropy that can be contained within a finite region of space with a given amount of energy.
-
D.
“The four laws of black hole mechanics”
“The four laws of black hole mechanics” is a foundational 1973 paper in theoretical physics that established the analogy between black hole dynamics and the laws of thermodynamics, laying the groundwork for black hole thermodynamics.
-
E.
Gibbons–Hawking temperature
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.
- 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_69ca848364f881908a24366a6feec1db |
completed | March 30, 2026, 2:11 p.m. |
| NER | Named-entity recognition | batch_69cdec011c24819089b456fc8b9ed80c |
completed | April 2, 2026, 4:09 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69d2e62c1984819095fcb239f11731b4 |
completed | April 5, 2026, 10:46 p.m. |
Created at: March 30, 2026, 9:08 p.m.