Triple
T7189120
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Saffman–Taylor instability |
E167641
|
entity |
| Predicate | discoveredBy |
P412
|
FINISHED |
| Object | Philip Geoffrey Saffman |
E31570
|
NE FINISHED |
Disambiguation candidates (1 decision)
The exact options the model was shown at each disambiguation step, with the option it chose highlighted — the evidence behind this triple's disambiguated ids.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Philip Geoffrey Saffman Context triple: [Saffman–Taylor instability, discoveredBy, Philip Geoffrey Saffman]
-
A.
Philip G. Saffman
chosen
Philip G. Saffman was a prominent British-American applied mathematician and fluid dynamicist known for his influential work on vortex dynamics and the theory of turbulence.
-
B.
Raymond E. Goldstein
Raymond E. Goldstein is a physicist renowned for his pioneering work in biological and nonlinear fluid dynamics, for which he received the APS Fluid Dynamics Prize.
-
C.
G. K. Batchelor
G. K. Batchelor was a prominent British applied mathematician and fluid dynamicist known for his foundational contributions to turbulence theory and for authoring the classic text "An Introduction to Fluid Dynamics."
-
D.
Geoffrey Smith
Geoffrey Smith is an Australian Anglican archbishop who serves as the national leader (Primate) of the Anglican Church of Australia.
-
E.
Michael S. Longuet-Higgins
Michael S. Longuet-Higgins was a British mathematician and oceanographer renowned for his influential work on wave theory and fluid dynamics.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (3 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69c6888b5248819090499a884ee3ec39 |
elicitation | completed |
| NER | batch_69c6e8e3d9188190ba2792098d76fb86 |
ner | completed |
| NED1 | batch_69c7bf903f1c819098de137c8c43ca34 |
ned_source_triple | completed |
Created at: March 27, 2026, 2:50 p.m.