Triple
T10147822
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | The four laws of black hole mechanics |
E231749
|
entity |
| Predicate | instanceOf |
P0
|
FINISHED |
| Object | foundational work in black hole thermodynamics |
C27492
|
CONCEPT FINISHED |
How this triple was built (1 step)
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.
CD
Concept disambiguation
gpt-5-mini-2025-08-07
Target class: foundational work in black hole thermodynamics Context triple: [The four laws of black hole mechanics, instanceOf, foundational work in black hole thermodynamics]
-
A.
black hole uniqueness theorem
The black hole uniqueness theorem states that any stationary, asymptotically flat black hole solution of the Einstein–Maxwell equations in four dimensions is completely characterized by only three externally observable parameters: mass, electric charge, and angular momentum.
-
B.
non-singular black hole model
A non-singular black hole model is a theoretical description of a black hole whose core avoids the classical spacetime singularity, typically by invoking modified gravity or quantum effects that yield a finite, regular interior geometry.
-
C.
formulation of cosmic censorship conjecture
The formulation of the cosmic censorship conjecture is the theoretical class of principles proposing that singularities arising from gravitational collapse are always hidden within event horizons, preventing "naked" singularities from being observed and thus preserving the predictability of general relativity.
-
D.
black hole model
A black hole model is a conceptual representation that describes the physical properties, structure, and behavior of black holes, including their formation, spacetime geometry, and interactions with surrounding matter and radiation.
-
E.
law of black-body radiation
The law of black-body radiation describes how an idealized object emits electromagnetic radiation with an intensity and spectrum that depend solely on its temperature, as quantified by Planck’s radiation formula.
- F. None of above. chosen
Provenance (1 batch)
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_69ca848364f881908a24366a6feec1db |
completed | March 30, 2026, 2:11 p.m. |
Created at: March 30, 2026, 9:08 p.m.