Triple

T20690525
Position Surface form Disambiguated ID Type / Status
Subject holographic principle E508537 entity
Predicate hasVariant P455 FINISHED
Object Bousso bound
The Bousso bound is a conjectured limit in theoretical physics that constrains the maximum entropy or information that can pass through certain light-like surfaces, refining the holographic principle in general spacetimes.
E1445857 NE FINISHED

How this triple was built (4 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: Bousso bound | Statement: [holographic principle, hasVariant, Bousso bound]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Bousso bound
Context triple: [holographic principle, hasVariant, Bousso bound]
  • A. Bekenstein bound
    The Bekenstein bound is a theoretical limit in physics on the maximum amount of information or entropy that can be contained within a finite region of space with a given amount of energy.
  • B. Bekenstein–Hawking entropy
    Bekenstein–Hawking entropy is the thermodynamic entropy associated with a black hole, proportional to the area of its event horizon and fundamental in linking gravity, quantum theory, and thermodynamics.
  • C. Buchdahl bound
    The Buchdahl bound is a theoretical limit in general relativity that constrains how compact a stable, spherically symmetric star can be before collapsing into a black hole.
  • D. Borde–Guth–Vilenkin theorem
    The Borde–Guth–Vilenkin theorem is a result in cosmology showing that any universe which has, on average, been expanding throughout its history must have a past boundary, implying that inflationary models cannot be eternal into the past.
  • E. Weyl curvature hypothesis
    The Weyl curvature hypothesis is Roger Penrose’s proposal that the universe began in an extremely low-gravitational-entropy, highly ordered state characterized by vanishing Weyl curvature, providing a geometric explanation for the cosmological arrow of time.
  • 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: Bousso bound
Triple: [holographic principle, hasVariant, Bousso bound]
Generated description
The Bousso bound is a conjectured limit in theoretical physics that constrains the maximum entropy or information that can pass through certain light-like surfaces, refining the holographic principle in general spacetimes.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Bousso bound
Target entity description: The Bousso bound is a conjectured limit in theoretical physics that constrains the maximum entropy or information that can pass through certain light-like surfaces, refining the holographic principle in general spacetimes.
  • A. Bekenstein bound
    The Bekenstein bound is a theoretical limit in physics on the maximum amount of information or entropy that can be contained within a finite region of space with a given amount of energy.
  • B. Bekenstein–Hawking entropy
    Bekenstein–Hawking entropy is the thermodynamic entropy associated with a black hole, proportional to the area of its event horizon and fundamental in linking gravity, quantum theory, and thermodynamics.
  • C. Buchdahl bound
    The Buchdahl bound is a theoretical limit in general relativity that constrains how compact a stable, spherically symmetric star can be before collapsing into a black hole.
  • D. Borde–Guth–Vilenkin theorem
    The Borde–Guth–Vilenkin theorem is a result in cosmology showing that any universe which has, on average, been expanding throughout its history must have a past boundary, implying that inflationary models cannot be eternal into the past.
  • E. Weyl curvature hypothesis
    The Weyl curvature hypothesis is Roger Penrose’s proposal that the universe began in an extremely low-gravitational-entropy, highly ordered state characterized by vanishing Weyl curvature, providing a geometric explanation for the cosmological arrow of time.
  • F. None of above. chosen

Provenance (5 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_69e0b4c1ed408190b72dd26b1e33f8a1 completed April 16, 2026, 10:06 a.m.
NER Named-entity recognition batch_69e6c10cb5588190acb88f2c82fc593a completed April 21, 2026, 12:13 a.m.
NED1 Entity disambiguation (via context triple) batch_6a08d7e226808190bf05b85afb173e36 completed May 16, 2026, 8:47 p.m.
NEDg Description generation batch_6a08d9ca43288190a2be3d4f63141391 completed May 16, 2026, 8:55 p.m.
NED2 Entity disambiguation (via description) batch_6a08da457ee48190ba18b3e34f117e19 completed May 16, 2026, 8:57 p.m.
Created at: April 16, 2026, 12:08 p.m.