A Simplified Treatment of Gravitational Interaction on Galactic Scales
Sascha Trippe (SNU Seoul)

TL;DR
This paper proposes a simplified, toy model for galactic-scale gravity based on massive gravitons, successfully reproducing key galactic phenomena without dark matter, but relies on ad-hoc assumptions and is not a complete theory.
Contribution
It introduces a novel scaling law for gravity on galactic scales using massive gravitons, explaining rotation curves and galaxy relations without dark matter.
Findings
Predicts flat galactic rotation curves
Reproduces Tully-Fisher and Faber-Jackson relations
Accounts for galaxy cluster kinematics
Abstract
I present a simple scheme for the treatment of gravitational interactions on galactic scales. In analogy to known mechanisms of quantum field theory, I assume ad hoc that gravitation is mediated by virtual exchange particles - gravitons - with very small but non-zero masses. The resulting density and mass profiles are proportional to the mass of the gravitating body. The mass profile scales with the centripetal acceleration experienced by a test particle orbiting the central mass; this comes at the cost of postulating a universal characteristic acceleration a0 = 4.3*10^{-12} m/s^2 (or 8*pi*a0 = 1.1*10^{-10} m/s^2). The scheme predicts the asymptotic flattening of galactic rotation curves, the Tully-Fisher/Faber-Jackson relations, the mass discrepancy-acceleration relation of galaxies, the surface brightness-acceleration relation of galaxies, the kinematics of galaxy clusters, and…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
