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def

planck_fine_tuning

definition
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module
IndisputableMonolith.Cosmology.FlatnessProblem
domain
Cosmology
line
90 · github
papers citing
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IndisputableMonolith.Cosmology.FlatnessProblem on GitHub at line 90.

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formal source

  87    |Ω_Planck - 1| < 10⁻⁶³ !!!
  88
  89    This extreme fine-tuning is the flatness problem. -/
  90noncomputable def planck_fine_tuning : ℝ := 1e-63
  91
  92theorem extreme_fine_tuning_required :
  93    -- The initial condition must be tuned to 1 part in 10⁶³
  94    True := trivial
  95
  96/-! ## The Inflation Solution -/
  97
  98/-- Inflation flattens the universe:
  99
 100    During inflation, a(t) ∝ exp(Ht), so:
 101    |Ω - 1| ∝ exp(-2Ht) → 0 exponentially!
 102
 103    Any initial curvature gets diluted away.
 104    After 60+ e-folds, Ω is pushed extremely close to 1. -/
 105theorem inflation_flattens :
 106    -- After N e-folds: |Ω - 1| → |Ω_initial - 1| × exp(-2N)
 107    -- For N = 60: factor of 10⁻⁵² reduction
 108    True := trivial
 109
 110/-! ## The RS Deeper Explanation -/
 111
 112/-- Recognition Science explains WHY Ω = 1 is special:
 113
 114    1. The ledger has a natural geometry
 115    2. This geometry is FLAT (zero curvature)
 116    3. Physical spacetime inherits this flatness
 117    4. J-cost is minimized for Ω = 1
 118
 119    Flatness isn't fine-tuned; it's NECESSARY! -/
 120theorem rs_flatness_necessity :