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.