Scale-Invariant Dynamics of Galaxies, MOND, Dark Matter, and the Dwarf Spheroidals
arXiv:2001.04978 · doi:10.1093/mnras/stz3613
Abstract
The Scale-Invariant Vacuum (SIV) theory is based on Weyl's Integrable Geometry, endowed with a gauge scalar field. The main difference between MOND and the SIV theory is that the first considers a global dilatation invariance of space and time, where the scale factor is a constant, while the second opens the likely possibility that is a function of time. The key equations of the SIV framework are used here to study the relationship between the Newtonian gravitational acceleration due to baryonic matter and the observed kinematical acceleration . The relationship is applied to galactic systems of the same age where the Radial Acceleration Relation (RAR), between the and accelerations, can be compared with observational data. The SIV theory shows an excellent agreement with observations and with MOND for baryonic gravities m s. Below this value, SIV still fully agrees with the observations, as well as with the horizontal asymptote of the RAR for dwarf spheroidals, while this is not the case for MOND. These results support the view that there is no need for dark matter and that the RAR and related dynamical properties of galaxies can be interpreted by a modification of gravitation.
12 pages, 3 figures
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Cited by in corpus (10)
- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- Strong constraints on the gravitational law from DR3 wide binaries
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