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arXiv · 1707.01619

Galaxy rotation curves and the deceleration parameter in weak gravity

Maurice H. P. M. van Putten
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Abstract

We present a theory of weak gravity parameterized by a fundamental frequency $ω_0 = \sqrt{1-q}H$ of the cosmoloogical horizon, where $H$ and $q$ denote the Hubble and, respectively, deceleration parameter. It predicts (i) a $C^0$ onset to weak gravity across accelerations $α= a_{dS}$ in galaxy rotation curves, where $a_{dS}=cH$ denotes the de Sitter acceleration with velocity of light $c$, and (ii) fast evolution $Q(z)=dq(z)/dz$ of the deceleration parameter by $Λ=ω_0^2$ satisfying $Q_0>2.5$, $Q_0=Q(0)$, distinct from $Q_0\lesssim1$ in $Λ$CDM. The first is identified in high resolution data of Lellie et al.(2017), the second in heterogeneous data on $H(z)$ over $0<z<2$. A model-independent cubic fit in the second rules out $Λ$CDM by $4.35σ$ and obtains $H_0=74.0\pm 2.2$ km s$^{-1}$ Mpc$^{-1}$ consistent with Riess et al. (2016). Comments on possible experimental tests by the LISA Pathfinder are included.

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Maurice H. P. M. van Putten. 2017-07-06. Galaxy rotation curves and the deceleration parameter in weak gravity. https://doi.org/10.1142/s0217732317300191

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