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.