Dark Matter Phase Transition Constrained at O(0.1) eV with LSB Rotation Curves
Jorge Mastache, Axel de la Macorra, Jorge L. Cervantes-Cota

TL;DR
This paper introduces a particle-physics motivated dark matter model called BDM, which predicts a phase transition at about 0.06 eV, and fits galaxy rotation curves to constrain this transition and core parameters.
Contribution
The paper proposes a new dark matter model with a phase transition scale Ec and constrains it using galaxy rotation curves, providing a fundamental particle physics scale.
Findings
Average core radius rc = 1.48 kpc
Transition energy Ec = 0.06 eV
Cored profiles are favored over cuspy profiles
Abstract
In order to unravel the nature of the dark matter (DM) we have proposed a particle-physics motivated model called Bound Dark Matter (BDM) that consist in DM massless particles above a threshold energy Ec that acquire mass below it due to nonperturbative methods. Therefore, the BDM model describes DM particles which are relativistic, hot dark matter (HDM) in the denser (inner) regions of galaxies and describes nonrelativistic, cold dark matter (CDM) where halo density is below rho_c = Ec^4. We test this model by fitting rotation curves from Low Surface Brightness (LSB) galaxies from The HI Nearby Galaxy Survey (THINGS). We use a particular DM cored profile that contains three parameters: a typical scale length (rs) and density (rho_0) of the halo, and a core radius (rc) stemming from the relativistic nature of the BDM model. Since the energy Ec parameterizes the phase transition due to…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena
