Triple

T1986334
Position Surface form Disambiguated ID Type / Status
Subject Kerr–Newman black hole E43148 entity
Predicate hasThermodynamicProperty P23698 FINISHED
Object Hawking temperature
Hawking temperature is the characteristic black-body radiation temperature associated with black holes, arising from quantum effects near the event horizon and determining the rate at which they evaporate.
E26863 NE FINISHED

How this triple was built (5 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: Hawking temperature | Statement: [Kerr–Newman black hole, hasThermodynamicProperty, Hawking temperature]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Hawking temperature
Context triple: [Kerr–Newman black hole, hasThermodynamicProperty, Hawking temperature]
  • A. Gibbons–Hawking temperature
    The Gibbons–Hawking temperature is the characteristic thermal radiation temperature associated with the cosmological horizon of de Sitter space, analogous to the Hawking temperature of black holes.
  • B. Hawking radiation
    Hawking radiation is the theoretical blackbody radiation predicted to be emitted by black holes due to quantum effects near the event horizon, causing them to lose mass and eventually evaporate.
  • C. 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.
  • D. Planck temperature
    The Planck temperature is the theoretical maximum meaningful temperature in physics, above which current physical theories, including quantum mechanics and general relativity, are expected to break down.
  • E. 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.
  • 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: Hawking temperature
Triple: [Kerr–Newman black hole, hasThermodynamicProperty, Hawking temperature]
Generated description
Hawking temperature is the characteristic black-body radiation temperature associated with black holes, arising from quantum effects near the event horizon and determining the rate at which they evaporate.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Hawking temperature
Target entity description: Hawking temperature is the characteristic black-body radiation temperature associated with black holes, arising from quantum effects near the event horizon and determining the rate at which they evaporate.
  • A. Gibbons–Hawking temperature
    The Gibbons–Hawking temperature is the characteristic thermal radiation temperature associated with the cosmological horizon of de Sitter space, analogous to the Hawking temperature of black holes.
  • B. Hawking radiation chosen
    Hawking radiation is the theoretical blackbody radiation predicted to be emitted by black holes due to quantum effects near the event horizon, causing them to lose mass and eventually evaporate.
  • C. 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.
  • D. Planck temperature
    The Planck temperature is the theoretical maximum meaningful temperature in physics, above which current physical theories, including quantum mechanics and general relativity, are expected to break down.
  • E. 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.
  • F. None of above.
PD Predicate disambiguation gpt-5-mini-2025-08-07
Target predicate: hasThermodynamicProperty
Context triple: [Kerr–Newman black hole, hasThermodynamicProperty, Hawking temperature]
  • A. hasTemperature
    Indicates that an entity possesses or is characterized by a specific temperature value.
  • B. thermalConductivity
    Indicates how effectively heat is conducted through a material per unit temperature gradient.
  • C. measuredProperty
    Indicates that the subject is a measurement that quantifies or assesses the specified property of an entity.
  • D. haveProperty chosen
    Indicates that an entity possesses, exhibits, or is characterized by a particular property or attribute.
  • E. thermalExpansionCoefficient
    Indicates how much a material's size changes per unit length (or volume) for each degree change in temperature.
  • F. None of above.

Provenance (6 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_69a88713ddc88190a969715658ebe7a8 completed March 4, 2026, 7:25 p.m.
NER Named-entity recognition batch_69abb96f932881908bebfc4176fda7c0 completed March 7, 2026, 5:36 a.m.
NED1 Entity disambiguation (via context triple) batch_69ae0331eec881909463163fb71e4eba completed March 8, 2026, 11:16 p.m.
NEDg Description generation batch_69ae03e575a88190a93181eb9d9bc3eb completed March 8, 2026, 11:19 p.m.
NED2 Entity disambiguation (via description) batch_69ae0473aecc8190b3da07fb8fd18e81 completed March 8, 2026, 11:21 p.m.
PD Predicate disambiguation batch_69abb798d288819083132cf14605bd02 completed March 7, 2026, 5:28 a.m.
Created at: March 4, 2026, 7:37 p.m.