Scalar field: free field , frozen field
ProvedCosmologyEOS.scalar_field_limiting_casescosmologymathematical-physics
For a homogeneous scalar field with time derivative and potential energy , the equation of state is . Then:
- a free field () with has ;
- a field with vanishing kinetic energy () and has , i.e. it is equivalent to a cosmological constant.
Preamble
import Mathlib import Definitions.Def_CosmologyEOS_Defs open Real Filter Topology
Formal statement
namespace CosmologyEOS
theorem scalar_field_limiting_cases :
(∀ phiDot : ℝ, phiDot ≠ 0 → scalarFieldEOS phiDot 0 = 1) ∧
(∀ V : ℝ, V ≠ 0 → scalarFieldEOS 0 V = -1) := by
sorry
end CosmologyEOSSource
Wikipedia, "Equation of state (cosmology)", revision 1375011367, https://en.wikipedia.org/w/index.php?title=Equation_of_state_(cosmology)&oldid=1375011367, section 'Scalar modeling'
Read-back
What the Lean code literally says, in plain math · Aristotle (Harmonic) — same agent as the drafter; NON-BLIND
NON-BLIND READ-BACK — NOT INDEPENDENT TESTIMONY. This read-back was written by the same agent that drafted the Lean statement below, with full knowledge of the source text and of the intended meaning. It was not produced by a blind, independent auditor, so it must not be mistaken for independent testimony; reviewers should compare the Lean code with the source themselves.
With (value when the denominator is ), the statement asserts both: (1) for every real , ; (2) for every real , .
Human review