Triple
T6859165
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | On the Law of Distribution of Energy in the Normal Spectrum |
E158227
|
entity |
| Predicate | mainSubject |
P3
|
FINISHED |
| Object | Planck radiation law |
E4994
|
NE FINISHED |
Named-entity recognition
Before disambiguation, gpt-5-mini classified whether the object phrase is a named entity — the step behind the object's NE type shown above.
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: Planck radiation law | Statement: [On the Law of Distribution of Energy in the Normal Spectrum, mainSubject, Planck radiation law]
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: Planck radiation law Context triple: [On the Law of Distribution of Energy in the Normal Spectrum, mainSubject, Planck radiation law]
-
A.
Planck radiation law
chosen
Planck radiation law is a fundamental formula in quantum physics that describes the spectral distribution of electromagnetic radiation emitted by a black body in thermal equilibrium.
-
B.
Wien displacement law
Wien's displacement law is a physical law that relates the temperature of a blackbody to the wavelength at which it emits radiation most intensely.
-
C.
Stefan–Boltzmann law
The Stefan–Boltzmann law is a fundamental principle of thermal radiation stating that the total energy radiated per unit surface area of a black body is proportional to the fourth power of its absolute temperature.
-
D.
Kirchhoff's law of thermal radiation
Kirchhoff's law of thermal radiation is a fundamental principle in thermodynamics stating that, for a body in thermal equilibrium, its emissivity equals its absorptivity at each wavelength.
-
E.
Wien displacement constant
The Wien displacement constant is the proportionality constant that relates the temperature of a black body to the wavelength at which it emits radiation most intensely.
- 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_69c68830cdbc8190a8301c7a9d9f651a |
elicitation | completed |
| NER | batch_69c6d8720bd48190adb446130a03d2bf |
ner | completed |
| NED1 | batch_69c74283a6e0819090366d8d677ed4fa |
ned_source_triple | completed |
Created at: March 27, 2026, 2:21 p.m.