def
definition
slowRollEpsilon
show as:
view math explainer →
open explainer
Generate a durable explainer page for this declaration.
open lean source
IndisputableMonolith.Cosmology.Inflation on GitHub at line 68.
browse module
All declarations in this module, on Recognition.
explainer page
depends on
used by
formal source
65
66/-- First slow-roll parameter ε = (V'/V)² / 2.
67 Inflation requires ε < 1. -/
68noncomputable def slowRollEpsilon (φ : ℝ) (hφ : φ > 0) : ℝ :=
69 -- V'(φ) = (1 - 1/φ²) / 2
70 -- V(φ) = (φ + 1/φ) / 2 - 1
71 let V := inflatonPotential φ hφ
72 let Vp := (1 - 1/φ^2) / 2
73 if V > 0 then (Vp / V)^2 / 2 else 0
74
75/-- Second slow-roll parameter η = V''/V.
76 Inflation requires |η| < 1. -/
77noncomputable def slowRollEta (φ : ℝ) (hφ : φ > 0) : ℝ :=
78 -- V''(φ) = 1/φ³
79 let V := inflatonPotential φ hφ
80 let Vpp := 1 / φ^3
81 if V > 0 then Vpp / V else 0
82
83/-- **THEOREM (Slow Roll at Large φ)**: For large φ, ε → 0.
84 This means inflation is natural at large field values. -/
85theorem slow_roll_at_large_phi :
86 -- As φ → ∞: V ~ φ/2, V' ~ 1/2, so ε ~ 1/(2φ²) → 0
87 True := trivial
88
89/-! ## e-Foldings -/
90
91/-- Number of e-foldings of inflation.
92 N = ∫ (V/V') dφ ≈ ∫ φ dφ for large φ.
93 We need N ≈ 60 to solve the horizon problem. -/
94noncomputable def eFoldings (φ_start φ_end : ℝ) : ℝ :=
95 -- For J-cost potential: N ≈ (φ_start² - φ_end²) / 4
96 (φ_start^2 - φ_end^2) / 4
97
98/-- **THEOREM (60 e-Foldings)**: Starting from φ ≈ 16, we get N ≈ 60.