A Preference for Cold Dark Matter over Superfluid Dark Matter in Local Milky Way Data

Abstract

There are many well-known correlations between dark matter and baryons that exist on galactic scales. These correlations can essentially be encompassed by a simple scaling relation between observed and baryonic accelerations, historically known as the Mass Discrepancy Acceleration Relation (MDAR). The existence of such a relation has prompted many theories that attempt to explain the correlations by invoking additional fundamental forces on baryons. The standard lore has been that a theory that reduces to the MDAR on galaxy scales but behaves like cold dark matter (CDM) on larger scales provides an excellent fit to data, since CDM is desirable on scales of clusters and above. However, this statement should be revised in light of recent results showing that a fundamental force that reproduces the MDAR is challenged by local Milky Way dynamics and rotation curve data between 5-18 kpc. In this study, we test this claim on the example of Superfluid Dark Matter. We find that a standard CDM model is preferred over a static superfluid profile assuming a steady-state Galactic disk and discuss the robustness of this conclusion to disequilibrium effects. This preference is due to the fact that the superfluid model over-predicts vertical accelerations, even while reproducing galactic rotation curves. Our results establish an important criterion that any dark matter model must satisfy within the Milky Way.

6 pages, 2 figures, 3 appendices; updated to match published version (v2)

References in corpus (17)

• galpy: A Python Library for Galactic Dynamics
• The Radial Acceleration Relation in Rotationally Supported Galaxies
• A dynamically young and perturbed Milky Way disk
• Vertical waves in the solar neighbourhood in Gaia DR2
• The Circular Velocity Curve of the Milky Way from $5$ to $25$ kpc
• Footprints of the Sagittarius dwarf galaxy in the $Gaia$ data set
• The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry and location
• MOND theory
• Gravitational polarization and the phenomenology of MOND
• Phenomenological consequences of superfluid dark matter with baryon-phonon coupling
• Kinematics with Gaia DR2: The Force of a Dwarf
• Reconciling MOND and dark matter?
• Galactoseismology and the Local Density of Dark Matter
• Implications of a time-varying Galactic potential for determinations of the dynamical surface density
• Dynamical Friction in Superfluids
• The Radial Acceleration Relation (RAR): the crucial cases of Dwarf Discs and of Low Surface Brightness galaxies
• The Imprint of Spiral Arms on the Galactic Rotation Curve