Einstein's static universe (eq. 10):
ProvedCosmoConstCentury.einstein_static_universe_iffLet and be constants, and let , , be arbitrary real constants with . The constant scale factor together with the constant density solves the closed () Friedmann–Lemaître dust equations (15)–(16) for all times if and only if
In units with this is Einstein's 1917 relation (10), , linking the cosmological constant, the mean density and the radius of the static closed universe.
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 .
import Mathlib import Definitions.Def_CosmoConstCentury_Defs open Filter Topology
namespace CosmoConstCentury
theorem einstein_static_universe_iff (G c Λ R₀ ρ₀ : ℝ) (hR₀ : 0 < R₀) :
IsFriedmannSolution G c Λ 1 Set.univ (fun _ => R₀) (fun _ => ρ₀) ↔
(Λ = einsteinKappa G c * c ^ 2 * ρ₀ / 2 ∧ Λ = 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 sign conditions on , , , ). Write (which is if ). The statement asserts the equivalence of:
- the constant functions and form a Friedmann solution with curvature index on the whole real line, i.e. for every real : , is near , and (since )
- and .