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rs_omega_m_h2
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IndisputableMonolith.Physics.BAO on GitHub at line 73.
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70def rs_omega_b_h2 : ℝ := 0.022
71
72/-- **RS MATTER DENSITY**: Ω_m h² ≈ 0.143 from RS dark matter + baryons. -/
73def rs_omega_m_h2 : ℝ := 0.143
74
75/-- Matter density exceeds baryon density (dark matter component). -/
76theorem matter_exceeds_baryons : rs_omega_b_h2 < rs_omega_m_h2 := by
77 norm_num [rs_omega_b_h2, rs_omega_m_h2]
78
79/-- **RS SPECTRAL INDEX**: n_s ≈ 0.967 from slow-roll inflation.
80 n_s = 1 - 2/N_e where N_e ≈ 60 e-foldings. -/
81noncomputable def rs_spectral_index (N_e : ℝ) : ℝ := 1 - 2 / N_e
82
83/-- For N_e = 60 e-foldings: n_s ≈ 0.967. -/
84theorem spectral_index_60efolds :
85 rs_spectral_index 60 = 1 - 1/30 := by
86 unfold rs_spectral_index
87 norm_num
88
89/-- Spectral index is less than 1 (red-tilted spectrum). -/
90theorem spectral_index_red_tilt (N_e : ℝ) (hN : 0 < N_e) :
91 rs_spectral_index N_e < 1 := by
92 unfold rs_spectral_index
93 linarith [div_pos two_pos hN]
94
95/-! ## Sound Horizon -/
96
97/-- **RS DRAG EPOCH REDSHIFT**: z_drag ≈ 1060.
98 This is where baryons decouple from photons (Saha equation). -/
99def rs_drag_redshift : ℝ := 1060
100
101/-- **SOUND HORIZON** (simplified formula valid for matter+radiation):
102 r_s ≈ (2/3) × (c / k_eq) × √(6/R_eq) × ln[...]
103 where k_eq is the wavenumber at matter-radiation equality.