Triple

T9937856
Position Surface form Disambiguated ID Type / Status
Subject cosmic censorship conjecture E194000 entity
Predicate relatedTo P37 FINISHED
Object no-hair theorem E6813 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: no-hair theorem | Statement: [cosmic censorship conjecture, relatedTo, no-hair theorem]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: no-hair theorem
Context triple: [cosmic censorship conjecture, relatedTo, no-hair theorem]
  • A. black hole no-hair theorem chosen
    The black hole no-hair theorem is a principle in general relativity stating that stationary black holes are completely characterized by only a few macroscopic parameters—mass, electric charge, and angular momentum—regardless of the details of the matter that formed them.
  • B. cosmic no-hair conjecture
    The cosmic no-hair conjecture is a theoretical proposal in cosmology stating that, under broad conditions, an expanding universe with a positive cosmological constant will evolve toward a homogeneous, isotropic de Sitter–like state, effectively erasing most information about its initial conditions.
  • C. cosmic censorship conjecture
    The cosmic censorship conjecture is a hypothesis in general relativity proposing that singularities arising from gravitational collapse are always hidden within event horizons, preventing "naked" singularities from being observed.
  • D. Schwarzschild black hole
    A Schwarzschild black hole is the simplest theoretical black hole solution in general relativity, describing a static, spherically symmetric, non-rotating, uncharged mass with an event horizon defined by the Schwarzschild radius.
  • E. Bardeen black hole model
    The Bardeen black hole model is a theoretical proposal of a regular (non-singular) black hole solution in general relativity that avoids the central singularity by coupling gravity to nonlinear electrodynamics.
  • 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_69ca82e409348190a393777356b80a2a completed March 30, 2026, 2:04 p.m.
NER Named-entity recognition batch_69cdb5e64760819094f599f158d32f33 completed April 2, 2026, 12:18 a.m.
NED1 Entity disambiguation (via context triple) batch_69d228f259b081909ce8a90ec1adad0d completed April 5, 2026, 9:18 a.m.
Created at: March 30, 2026, 8:44 p.m.