Another Path for the Emergence of Modified Galactic Dynamics from Dark Matter Superfluidity

TL;DR

This paper introduces an alternative mechanism for deriving Modified Newtonian Dynamics (MOND) from dark matter superfluidity by employing higher-gradient corrections, which modify gravity at galactic scales while preserving standard cosmological behavior.

Contribution

It proposes a novel approach using higher-gradient terms and symmetry breaking to derive MOND phenomenology from dark matter superfluidity, differing from previous phonon-mediated models.

Findings

The model reproduces MOND behavior at galactic scales.

Cosmological evolution remains consistent with LambdaCDM.

The mechanism involves spontaneous symmetry breaking depending on acceleration.

Abstract

In recent work we proposed a novel theory of dark matter (DM) superfluidity that matches the successes of the LambdaCDM model on cosmological scales while simultaneously reproducing MOdified Newtonian Dynamics (MOND) phenomenology on galactic scales. The agents responsible for mediating the MONDian force law are superfluid phonons that couple to ordinary (baryonic) matter. In this paper we propose an alternative way for the MOND phenomenon to emerge from DM superfluidity. The central idea is to use higher-gradient corrections in the superfluid effective theory. These next-to-leading order terms involve gradients of the gravitational potential, and therefore effectively modify the gravitational force law. In the process we discover a novel mechanism for generating the non-relativistic MOND action, starting from a theory that is fully analytic in all field variables. The idea, inspired by the symmetron mechanism, uses the spontaneous breaking of a discrete symmetry. For large acceleration, the symmetry is unbroken and the action reduces to Einstein gravity. For small acceleration, the symmetry is spontaneously broken and the action reduces to MONDian gravity. Cosmologically, however, the universe is always in the Einstein-gravity, symmetry-restoring phase. The expansion history and linear growth of density perturbations are therefore indistinguishable from LambdaCDM cosmology.