Triple
T10147832
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | The four laws of black hole mechanics |
E231749
|
entity |
| Predicate | mainSubject |
P3
|
FINISHED |
| Object |
black hole thermodynamics
Black hole thermodynamics is the field of theoretical physics that studies black holes using the concepts and laws of thermodynamics, relating quantities like entropy, temperature, and energy to their geometric and gravitational properties.
|
E231749
|
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 thermodynamics | Statement: [The four laws of black hole mechanics, mainSubject, black hole thermodynamics]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: black hole thermodynamics Context triple: [The four laws of black hole mechanics, mainSubject, black hole thermodynamics]
-
A.
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.
-
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.
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.
-
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. 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 thermodynamics Triple: [The four laws of black hole mechanics, mainSubject, black hole thermodynamics]
Generated description
Black hole thermodynamics is the field of theoretical physics that studies black holes using the concepts and laws of thermodynamics, relating quantities like entropy, temperature, and energy to their geometric and gravitational properties.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: black hole thermodynamics Target entity description: Black hole thermodynamics is the field of theoretical physics that studies black holes using the concepts and laws of thermodynamics, relating quantities like entropy, temperature, and energy to their geometric and gravitational properties.
-
A.
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.
-
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.
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.
-
D.
“The four laws of black hole mechanics”
chosen
“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.
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_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. |
| NEDg | Description generation | batch_69d2e73fd6988190a338a9e49dc3671b |
completed | April 5, 2026, 10:50 p.m. |
| NED2 | Entity disambiguation (via description) | batch_69d2e8c9058c8190bfa5720397331fa1 |
completed | April 5, 2026, 10:57 p.m. |
Created at: March 30, 2026, 9:08 p.m.