De Sitter's empty "Solution B" (eq. 13): ,
ProvedCosmoConstCentury.de_sitter_solution_B_iffLet and let , , be real constants. Consider the empty universe () with scale factor
This pair solves the closed () Friedmann–Lemaître dust equations (15)–(16) for all times if and only if
In units with this is de Sitter's 1917 "Solution B", , (13), written in the closed slicing in which de Sitter space appears as a Friedmann universe of minimal radius .
Formalization Note The predicate IsFriedmannSolution G c Λ k I R ρ requires, at every , that , that is in a neighbourhood of , and that the two equations hold with . De Sitter's original static coordinates are not used; the cosh form is the representation of the same empty solution in the closed Friedmann slicing.
import Mathlib import Definitions.Def_CosmoConstCentury_Defs open Filter Topology
namespace CosmoConstCentury
theorem de_sitter_solution_B_iff (G c Λ R₀ : ℝ) (hR₀ : 0 < R₀) :
IsFriedmannSolution G c Λ 1 Set.univ (fun t => R₀ * Real.cosh (c * t / R₀)) (fun _ => 0) ↔
Λ = 3 * c ^ 2 / R₀ ^ 2 := by sorry
end CosmoConstCenturyRead-back
What the Lean code literally says, in plain math · Aristotle (Harmonic)
Disclosure: non-blind read-back. This read-back was written by the same agent that drafted the Lean statement (Aristotle, by Harmonic), at the explicit request of the proposal owner. It is not an independent or blind audit, and it must not be treated as independent testimony: its author knew the source paper and the intended meaning while writing it. Reviewers should compare it against the Lean code themselves.
Let be real numbers with (no conditions on , , ). The statement asserts the equivalence of:
- the functions and form a Friedmann solution with on the whole real line: for every real , , is near , and
(the right side of the first equation is ); 2. .
Because the density is identically zero, plays no role. If the scale factor is the constant and condition 2 reads .
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.