Triple

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).

Phrase: Friedmann–Lemaître–Robertson–Walker metric | Statement: [Bardeen potential, appliesTo, Friedmann–Lemaître–Robertson–Walker metric]

Target entity: Friedmann–Lemaître–Robertson–Walker metric
Context triple: [Bardeen potential, appliesTo, Friedmann–Lemaître–Robertson–Walker metric]

• A. Lemaître–Tolman metric
  The Lemaître–Tolman metric is an exact spherically symmetric, inhomogeneous solution of Einstein’s field equations used in cosmology to model non-uniform distributions of matter without assuming spatial homogeneity.
• B. FLRW cosmological models chosen
  FLRW cosmological models are a family of solutions to Einstein’s field equations that describe a homogeneous and isotropic expanding or contracting universe, forming the standard framework for modern cosmology.
• C. Milne universe model
  The Milne universe model is a cosmological model that describes an empty, expanding universe with negative spatial curvature, serving as a special-relativistic alternative to general relativistic cosmologies.
• D. Gödel metric
  The Gödel metric is a solution to Einstein's field equations that describes a rotating universe allowing for closed timelike curves and thus the theoretical possibility of time travel.
• E. Lemaître–Hubble law
  The Lemaître–Hubble law is the fundamental cosmological relation that expresses the proportionality between a galaxy’s recessional velocity and its distance, providing the first observational evidence for the expansion of the universe.
• F. None of above.
• G. Unsure - the case is ambiguous/there is not enough information to decide.