Triple

T21988957
Position Surface form Disambiguated ID Type / Status
Subject Sakharov conditions E543034 entity
Predicate describedIn P519 FINISHED
Object Baryon asymmetry of the universe paper (1967)
The 1967 "Baryon asymmetry of the universe" paper is Andrei Sakharov’s seminal work that introduced the conditions required in the early universe to generate the observed matter–antimatter imbalance.
E1512259 NE FINISHED

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.

NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Baryon asymmetry of the universe paper (1967)
Context triple: [Sakharov conditions, describedIn, Baryon asymmetry of the universe paper (1967)]
  • A. Kobayashi–Maskawa paper on CP violation (1973)
    The Kobayashi–Maskawa paper on CP violation (1973) is a landmark theoretical work that extended the quark model to three generations, providing the mechanism for CP violation in the Standard Model and later underpinning the Nobel Prize in Physics for its authors.
  • B. Affleck–Dine baryogenesis scenarios
    Affleck–Dine baryogenesis scenarios are theoretical models in cosmology and particle physics that explain the universe’s matter–antimatter asymmetry via the dynamics of scalar fields carrying baryon number in the early universe.
  • C. Alpher–Bethe–Gamow paper
    The Alpher–Bethe–Gamow paper is a landmark 1948 cosmology paper that introduced the theory of Big Bang nucleosynthesis, explaining the origin of the light elements in the early universe.
  • D. “Synthesis of the Elements in Stars” (B2FH, 1957)
    “Synthesis of the Elements in Stars” (B2FH, 1957) is a landmark astrophysics paper that explained how chemical elements are formed through nuclear processes inside stars, laying the foundation for modern nucleosynthesis theory.
  • E. Fermi theory of beta decay
    The Fermi theory of beta decay is Enrico Fermi’s pioneering quantum field theory model that explains beta decay as a weak interaction process mediated by a four-fermion contact interaction, laying the groundwork for modern weak interaction theory.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg Description generation gpt-5.1
Instruction
Generate a one-sentence description of the target entity. 
You are given a context triple in the form (subject, predicate, object), where the object is the target entity. 
# Instructions
Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. 
Avoid repeating the information from the triple, unless really essential.
# Response Format
Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: Baryon asymmetry of the universe paper (1967)
Triple: [Sakharov conditions, describedIn, Baryon asymmetry of the universe paper (1967)]
Generated description
The 1967 "Baryon asymmetry of the universe" paper is Andrei Sakharov’s seminal work that introduced the conditions required in the early universe to generate the observed matter–antimatter imbalance.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Baryon asymmetry of the universe paper (1967)
Target entity description: The 1967 "Baryon asymmetry of the universe" paper is Andrei Sakharov’s seminal work that introduced the conditions required in the early universe to generate the observed matter–antimatter imbalance.
  • A. Kobayashi–Maskawa paper on CP violation (1973)
    The Kobayashi–Maskawa paper on CP violation (1973) is a landmark theoretical work that extended the quark model to three generations, providing the mechanism for CP violation in the Standard Model and later underpinning the Nobel Prize in Physics for its authors.
  • B. Affleck–Dine baryogenesis scenarios
    Affleck–Dine baryogenesis scenarios are theoretical models in cosmology and particle physics that explain the universe’s matter–antimatter asymmetry via the dynamics of scalar fields carrying baryon number in the early universe.
  • C. Alpher–Bethe–Gamow paper
    The Alpher–Bethe–Gamow paper is a landmark 1948 cosmology paper that introduced the theory of Big Bang nucleosynthesis, explaining the origin of the light elements in the early universe.
  • D. “Synthesis of the Elements in Stars” (B2FH, 1957)
    “Synthesis of the Elements in Stars” (B2FH, 1957) is a landmark astrophysics paper that explained how chemical elements are formed through nuclear processes inside stars, laying the foundation for modern nucleosynthesis theory.
  • E. Fermi theory of beta decay
    The Fermi theory of beta decay is Enrico Fermi’s pioneering quantum field theory model that explains beta decay as a weak interaction process mediated by a four-fermion contact interaction, laying the groundwork for modern weak interaction theory.
  • F. None of above. chosen

Provenance (4 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_69e0c48136b081908831fa907cc02e18 completed April 16, 2026, 11:14 a.m.
NED1 Entity disambiguation (via context triple) batch_6a0a6d81c92481909a58757f929f904c completed May 18, 2026, 1:38 a.m.
NEDg Description generation batch_6a0a6e18d4f48190bfb917c9c9109ea5 completed May 18, 2026, 1:40 a.m.
NED2 Entity disambiguation (via description) batch_6a0a6ee56684819082d2001b2e817ed8 completed May 18, 2026, 1:44 a.m.
Created at: April 16, 2026, 8:05 p.m.