Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
Valentina Cesare

TL;DR
This paper explores alternative gravity theories, specifically MOND and Refracted Gravity, to explain galactic phenomena and cosmological coincidences without dark matter or dark energy, addressing challenges faced by the standard model.
Contribution
It compares and discusses the potential of MOND and Refracted Gravity as small-scale solutions to galactic and cosmological issues, highlighting their ability to naturally explain observed relations.
Findings
MOND successfully predicts galaxy rotation curves without dark matter.
Refracted Gravity introduces a density-dependent modification to gravity.
Both theories address the acceleration scale coincidence with the cosmological constant.
Abstract
General relativity and its Newtonian weak field limit are not sufficient to explain the observed phenomenology in the Universe, from the formation of large-scale structures to the dynamics of galaxies, with the only presence of baryonic matter. The most investigated cosmological model, the CDM, accounts for the majority of observations by introducing two dark components, dark energy and dark matter, which represent 95% of the mass-energy budget of the Universe. Nevertheless, the CDM model faces important challenges on the scale of galaxies. For example, some very tight relations between the properties of dark and baryonic matters in disk galaxies, such as the baryonic Tully-Fisher relation (BTFR), the mass discrepancy-acceleration relation (MDAR), and the radial acceleration relation (RAR), which see the emergence of the acceleration scale $a_0 \simeq 1.2 \times…
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