Examines jet alignment and flux inversion in AGN, suggesting a link to black hole mass.
First large-scale observational test of the MSFCM using LoTSS DR2 × Tempel 2014 (80,695 AGN–filament pairs). Global signal ⟨cos2δ⟩ = −0.031 at 12.5σ. Two-regime density transition at ρ=2.09 (14.6σ). Flux inversion at S_thresh=4.77 mJy provides direct evidence for Γ_eff ∝ M_BH (Paper II eq. 7), confirmed at Spearman ρ=+0.084 (p<10⁻¹²⁷).
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Ariel Fernando Martini (2026) studied this question.
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