MDO fluid conservation (14) is equivalent to the field equation (7)
ProvedMDOUnifiedCosmology.conservation_iff_field_eqcosmologymathematical-physics
Throughout, (units ), is the scale factor of the flat FLRW metric, is the Hubble function, is the time-dependent part of the MDO fermionic field, is its potential, are the energy density and pressure of the other matter components, and .
Let , be defined by Eqs. (10)–(11). Fix a time at which , , , are differentiable, is differentiable at , and . Then the MDO conservation equation (14),
holds at if and only if the field equation (7),
holds at . This is the paper's remark that Eq. (14) is equivalent to Eq. (7).
Formalization Note The condition is needed for the direction (14) (7); no Friedmann equation is assumed.
Preamble
import Mathlib import Definitions.Def_MDOUnifiedCosmology_model open MDOUnifiedCosmology Set
Formal statement
namespace MDOUnifiedCosmology
theorem conservation_iff_field_eq (κ : ℝ) (V : ℝ → ℝ) (a φ : ℝ → ℝ) (t : ℝ)
(ha : DifferentiableAt ℝ a t) (ha' : DifferentiableAt ℝ (deriv a) t) (ha0 : a t ≠ 0)
(hφ : DifferentiableAt ℝ φ t) (hφ' : DifferentiableAt ℝ (deriv φ) t)
(hV : DifferentiableAt ℝ V (φ t)) (hφdot : deriv φ t ≠ 0) :
MDOConservation κ V a φ t ↔ FieldEq κ V a φ t := 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. 3, Eqs. (7), (10), (11), (14) and the sentence "the Eq. (14) is obviously equivalent to the Eq. (7)"
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