Triple
T17225945
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Wolfgang Rindler |
E418113
|
entity |
| Predicate | knownFor |
P22
|
FINISHED |
| Object | Rindler horizon |
E590890
|
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: Rindler horizon | Statement: [Wolfgang Rindler, knownFor, Rindler horizon]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Rindler horizon Context triple: [Wolfgang Rindler, knownFor, Rindler horizon]
-
A.
Rindler horizon
chosen
The Rindler horizon is the observer-dependent boundary in spacetime beyond which a uniformly accelerating observer cannot receive signals, analogous to a black hole event horizon.
-
B.
Rindler wedge
The Rindler wedge is the region of spacetime accessible to a uniformly accelerated observer in special relativity, often used to analyze horizons and thermal effects like the Unruh effect.
-
C.
Rindler coordinates
Rindler coordinates are a coordinate system in special relativity adapted to uniformly accelerated observers, covering only part of Minkowski spacetime and revealing horizon-like structures relevant to phenomena such as the Unruh effect.
-
D.
Cauchy horizon
A Cauchy horizon is a lightlike boundary in certain spacetime solutions of general relativity, such as rotating black holes, beyond which the deterministic evolution from initial data breaks down.
-
E.
“Cosmological event horizons, thermodynamics, and particle creation”
“Cosmological event horizons, thermodynamics, and particle creation” is a seminal paper by Gary W. Gibbons that explores the thermodynamic properties and quantum particle production associated with cosmological event horizons in expanding universes.
- 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_69d886d779488190b131369541c04e7d |
completed | April 10, 2026, 5:12 a.m. |
| NER | Named-entity recognition | batch_69e42de1674c81909ca9e87fa9153640 |
completed | April 19, 2026, 1:20 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a01675cc70881909cf39b2e229f5d1e |
completed | May 11, 2026, 5:21 a.m. |
Created at: April 10, 2026, 5:38 a.m.