Triple
T13062155
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Hermann Bondi |
E329223
|
entity |
| Predicate | notableWork |
P4
|
FINISHED |
| Object |
Bondi mass
Bondi mass is a concept in general relativity that measures the total mass-energy of an isolated system as observed from null infinity, accounting for energy carried away by gravitational radiation.
|
E1017419
|
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: Bondi mass | Statement: [Hermann Bondi, notableWork, Bondi mass]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Bondi mass Context triple: [Hermann Bondi, notableWork, Bondi mass]
-
A.
Bondi–Metzner–Sachs symmetry
Bondi–Metzner–Sachs symmetry is an infinite-dimensional group of asymptotic spacetime symmetries in general relativity that characterizes the gravitational field at null infinity, especially in the context of gravitational radiation.
-
B.
Gibbons–Hawking–York boundary term
The Gibbons–Hawking–York boundary term is an additional term in the gravitational action of general relativity that ensures a well-defined variational principle in spacetimes with boundaries.
-
C.
Reissner–Nordström metric
The Reissner–Nordström metric is an exact solution in general relativity describing the spacetime geometry outside a static, spherically symmetric, electrically charged black hole.
-
D.
Buchdahl bound
The Buchdahl bound is a theoretical limit in general relativity that constrains how compact a stable, spherically symmetric star can be before collapsing into a black hole.
-
E.
Schwarzschild radius
The Schwarzschild radius is the critical distance from the center of a non-rotating, spherically symmetric mass at which its escape velocity equals the speed of light, defining the boundary of a black hole.
- 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: Bondi mass Triple: [Hermann Bondi, notableWork, Bondi mass]
Generated description
Bondi mass is a concept in general relativity that measures the total mass-energy of an isolated system as observed from null infinity, accounting for energy carried away by gravitational radiation.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Bondi mass Target entity description: Bondi mass is a concept in general relativity that measures the total mass-energy of an isolated system as observed from null infinity, accounting for energy carried away by gravitational radiation.
-
A.
Bondi–Metzner–Sachs symmetry
Bondi–Metzner–Sachs symmetry is an infinite-dimensional group of asymptotic spacetime symmetries in general relativity that characterizes the gravitational field at null infinity, especially in the context of gravitational radiation.
-
B.
Gibbons–Hawking–York boundary term
The Gibbons–Hawking–York boundary term is an additional term in the gravitational action of general relativity that ensures a well-defined variational principle in spacetimes with boundaries.
-
C.
Reissner–Nordström metric
The Reissner–Nordström metric is an exact solution in general relativity describing the spacetime geometry outside a static, spherically symmetric, electrically charged black hole.
-
D.
Buchdahl bound
The Buchdahl bound is a theoretical limit in general relativity that constrains how compact a stable, spherically symmetric star can be before collapsing into a black hole.
-
E.
Schwarzschild radius
The Schwarzschild radius is the critical distance from the center of a non-rotating, spherically symmetric mass at which its escape velocity equals the speed of light, defining the boundary of a black hole.
- 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_69d80771749c81909a6d9197b9504872 |
completed | April 9, 2026, 8:09 p.m. |
| NER | Named-entity recognition | batch_69d980e7ee548190b4b18bdb1357c359 |
completed | April 10, 2026, 10:59 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69f6cbe45c8c819080fbdf1d94376feb |
completed | May 3, 2026, 4:15 a.m. |
| NEDg | Description generation | batch_69f6cd3d5090819091b65f544ad139fd |
completed | May 3, 2026, 4:21 a.m. |
| NED2 | Entity disambiguation (via description) | batch_69f6cdc8d52c819083717a455d589646 |
completed | May 3, 2026, 4:23 a.m. |
Created at: April 9, 2026, 8:59 p.m.