Triple

T19652956
Position Surface form Disambiguated ID Type / Status
Subject Pais–Uhlenbeck oscillator E471861 entity
Predicate relatedTo P37 FINISHED
Object Ostrogradsky instability NE NERFINISHED

How this triple was built (3 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: Ostrogradsky instability | Statement: [Pais–Uhlenbeck oscillator, relatedTo, Ostrogradsky instability]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Ostrogradsky instability
Context triple: [Pais–Uhlenbeck oscillator, relatedTo, Ostrogradsky instability]
  • A. Nielsen–Olesen instability
    The Nielsen–Olesen instability is a quantum field theory phenomenon describing how certain uniform field configurations, such as constant chromomagnetic fields, become unstable and decay into more complex structures like flux tubes or vortices.
  • B. Chandrasekhar–Friedman–Schutz instability
    The Chandrasekhar–Friedman–Schutz instability is a gravitational-radiation-driven instability in rotating stars that can cause certain oscillation modes to grow by emitting gravitational waves.
  • C. Dolgov–Kawasaki stability condition in viable models
    The Dolgov–Kawasaki stability condition in viable models is a theoretical requirement in modified gravity ensuring that f(R) theories avoid tachyonic instabilities by demanding a positive second derivative of the gravitational action with respect to the Ricci scalar.
  • D. Bogoliubov–Parasyuk theorem
    The Bogoliubov–Parasyuk theorem is a fundamental result in quantum field theory that rigorously establishes a systematic procedure for renormalizing divergent Feynman diagrams.
  • E. Jeans instability
    Jeans instability is a gravitational phenomenon in astrophysics where regions within a gas cloud become unstable and collapse under their own gravity, leading to the formation of structures like stars and galaxies.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Ostrogradsky instability
Target entity description: Ostrogradsky instability is a fundamental problem in classical and quantum field theories with non-degenerate higher-derivative terms, leading to unbounded Hamiltonians and runaway solutions that render such theories physically unstable.
  • A. Nielsen–Olesen instability
    The Nielsen–Olesen instability is a quantum field theory phenomenon describing how certain uniform field configurations, such as constant chromomagnetic fields, become unstable and decay into more complex structures like flux tubes or vortices.
  • B. Chandrasekhar–Friedman–Schutz instability
    The Chandrasekhar–Friedman–Schutz instability is a gravitational-radiation-driven instability in rotating stars that can cause certain oscillation modes to grow by emitting gravitational waves.
  • C. Dolgov–Kawasaki stability condition in viable models
    The Dolgov–Kawasaki stability condition in viable models is a theoretical requirement in modified gravity ensuring that f(R) theories avoid tachyonic instabilities by demanding a positive second derivative of the gravitational action with respect to the Ricci scalar.
  • D. Bogoliubov–Parasyuk theorem
    The Bogoliubov–Parasyuk theorem is a fundamental result in quantum field theory that rigorously establishes a systematic procedure for renormalizing divergent Feynman diagrams.
  • E. Jeans instability
    Jeans instability is a gravitational phenomenon in astrophysics where regions within a gas cloud become unstable and collapse under their own gravity, leading to the formation of structures like stars and galaxies.
  • F. None of above. chosen

Provenance (2 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_69d8e51395348190ac1416d46dfc6db0 completed April 10, 2026, 11:54 a.m.
NER Named-entity recognition batch_69e6414327d88190826ab9511f2f8e48 completed April 20, 2026, 3:07 p.m.
Created at: April 10, 2026, 1:44 p.m.