Model of Dark Matter and Dark Energy Based on Gravitational Polarization
Luc Blanchet, Alexandre Le Tiec

TL;DR
This paper introduces a gravitational polarization model for dark matter and dark energy, showing it aligns with Lambda-CDM cosmology and reproduces MOND phenomenology at galactic scales, with a natural cosmological constant.
Contribution
It proposes a dipolar medium model within general relativity that unifies dark matter and dark energy and explains galactic dynamics without new particles.
Findings
Dipolar fluid mimics Lambda-CDM at cosmological scales.
Model reproduces MOND phenomenology at galactic scales.
Cosmological constant naturally arises from the model.
Abstract
A model of dark matter and dark energy based on the concept of gravitational polarization is investigated. We propose an action in standard general relativity for describing, at some effective or phenomenological level, the dynamics of a dipolar medium, i.e. one endowed with a dipole moment vector, and polarizable in a gravitational field. Using first-order cosmological perturbations, we show that the dipolar fluid is undistinguishable from standard dark energy (a cosmological constant Lambda) plus standard dark matter (a pressureless perfect fluid), and therefore benefits from the successes of the Lambda-CDM (Lambda-cold dark matter) scenario at cosmological scales. Invoking an argument of "weak clusterisation" of the mass distribution of dipole moments, we find that the dipolar dark matter reproduces the phenomenology of the modified Newtonian dynamics (MOND) at galactic scales. The…
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