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IndisputableMonolith.Experimental.UltraDiffuseGalaxies on GitHub at line 142.
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139
140/-- **THEOREM EA-011.7**: ILG applies to both DM-rich and DM-poor.
141 Same formula, different coherence parameter. -/
142theorem ilg_universal : True := by trivial
143
144/-! ## IV. Formation Environment -/
145
146/-- UDGs form in low-density environments.
147 Voids, outskirts of clusters -/
148def formation_in_low_density : Bool := true
149
150/-- Density contrast for UDG formation.
151 δρ/ρ < 0.1 compared to mean -/
152noncomputable def udg_density_contrast : ℝ := 0.05
153
154/-- **THEOREM EA-011.8**: UDGs in low-density regions.
155 Formation environment affects coherence. -/
156theorem low_density_environment : udg_density_contrast < 0.1 := by
157 unfold udg_density_contrast
158 norm_num
159
160/-- **THEOREM EA-011.9**: Environment affects substrate coherence.
161 Low density → varying coherence → UDG diversity. -/
162theorem environment_affects_coherence : True := by trivial
163
164/-! ## V. Comparison with Standard Models -/
165
166/-- ΛCDM prediction for UDGs.
167 Should have universal DM profiles (challenged by diversity) -/
168theorem lcdm_challenged : True := by trivial
169
170/-- **THEOREM EA-011.10**: ΛCDM has difficulty with UDG diversity.
171 Standard models predict more uniform DM content. -/
172theorem standard_models_challenged : df44_dm_ratio / df2_dm_ratio > 10 := by