Universal MOND relation between the baryonic and `dynamical' central surface densities of disc galaxies

preprint2016arXivOpen access

Abstract

I derive a new MOND relation for pure-disc galaxies: The `dynamical' central surface density, ΣD0Σ^0_D, deduced from the measured velocities, is a universal function of only the true, `baryonic' central surface density, ΣB0Σ^0_B: ΣD0=ΣMS(ΣB0/ΣM)Σ^0_D=Σ_M \mathcal{S}(Σ^0_B/Σ_M), where ΣM≡a0/2πGΣ_M\equiv a_0/2πG is the MOND surface density constant. This surprising result is shown to hold in both existing, nonrelativistic MOND theories. S(y)\mathcal{S}(y) is derived: S(y)=∫0yν(y′)dy′\mathcal{S}(y)=\int_0^yν(y')dy', with ν(y)ν(y) the interpolating function of the theory. The relation aymptotes to ΣD0=ΣB0Σ^0_D=Σ^0_B for ΣB0≫ΣMΣ^0_B\ggΣ_M, and to ΣD0=(4ΣMΣB0)1/2Σ^0_D=(4Σ_MΣ^0_B)^{1/2} for ΣB0≪ΣMΣ^0_B\llΣ_M. This study was prompted by the recent finding of a correlation between related attributes of disc galaxies by Lelli et al. (2016). The MOND central-surface-densities relation agrees very well with these results.

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