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MOND as a peculiar case of the SIV theory

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arxiv 2302.06206 v1 pith:6SG2J63P submitted 2023-02-13 gr-qc astro-ph.COastro-ph.GA

MOND as a peculiar case of the SIV theory

classification gr-qc astro-ph.COastro-ph.GA
keywords scaletheoryinvariantmondconstantcosmologicaldensitymatter
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The scale invariant theory is preserving the fundamental physical properties of General Relativity, while enlarging the group of invariances subtending gravitation theory (Dirac1973; Canuto et al.1977). The Scale Invariant Vacuum (SIV) theory assumes, as gauging condition, that:"The macroscopic empty space is scale invariant, homogeneous and isotropic". Some basic properties in Weyl's Integrable Geometry and cotensor calculus are examined in relation with scalar-tensor theories. Possible scale invariant effects are strongly reduced by matter density, both at the cosmological and local levels. The weak feld limit of SIV tends to MOND, when the scale factor is taken as constant, an approximation valid (<1%) over the last 400 Myr. A better understanding of the a0-parameter is obtained: it corresponds to the equilibrium point of the Newtonian and SIV dynamical acceleration. Parameter a0 is not a universal constant, it depends on the density and age of the Universe. As MOND is doing, SIV theory avoids the call to dark matter, moreover the cosmological models predict accelerated expansion.

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