Deceleration parameter , Eq. (31)
ProvedMDOUnifiedCosmology.deceleration_formulacosmologymathematical-physics
Let be a scale factor that is differentiable at with also differentiable at , and suppose and . With , the deceleration parameter satisfies
This is Eq. (31), used to analyse the phantom-like phase at the end of inflation and the reheating epoch.
Preamble
import Mathlib import Definitions.Def_MDOUnifiedCosmology_model open MDOUnifiedCosmology Set
Formal statement
namespace MDOUnifiedCosmology
theorem deceleration_formula (a : ℝ → ℝ) (t : ℝ) (ha : DifferentiableAt ℝ a t)
(ha' : DifferentiableAt ℝ (deriv a) t) (ha0 : a t ≠ 0) (had : deriv a t ≠ 0) :
decelerationParam a t = -1 - deriv (hubble a) t / hubble a t ^ 2 := by
sorry
end MDOUnifiedCosmologySource
S. H. Pereira, M. E. S. Alves, T. M. Guimarães, "An unified cosmological evolution driven by a mass dimension one fermionic field", Eur. Phys. J. C 79 (2019) 543, https://doi.org/10.1140/epjc/s10052-019-7036-5, p. 7, Eq. (31)
Human review
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.