Slowly rotating Bose Einstein Condensate galactic dark matter halos, and their rotation curves

Abstract

If dark matter is composed of massive bosons, a Bose-Einstein Condensation process must have occurred during the cosmological evolution. Therefore galactic dark matter may be in a form of a condensate, characterized by a strong self-interaction. We consider the effects of rotation on the Bose-Einstein Condensate dark matter halos, and we investigate how rotation might influence their astrophysical properties. In order to describe the condensate we use the Gross-Pitaevskii equation, and the Thomas-Fermi approximation, which predicts a polytropic equation of state with polytropic index $n=1$. By assuming a rigid body rotation for the halo, with the use of the hydrodynamic representation of the Gross-Pitaevskii equation we obtain the basic equation describing the density distribution of the rotating condensate. We obtain the general solutions for the condensed dark matter density, and we derive the general representations for the mass distribution, boundary (radius), potential energy, velocity dispersion, tangential velocity and for the logarithmic density and velocity slopes, respectively. Explicit expressions for the radius, mass, and tangential velocity are obtained in the first order of approximation, under the assumption of slow rotation. In order to compare our results with the observations we fit the theoretical expressions of the tangential velocity of massive test particles moving in rotating Bose-Einstein Condensate dark halos with the data of 12 dwarf galaxies, and the Milky Way, respectively.

22 pages, 7 figures, accepted for publication in EPJC

References in corpus (103)

• Planck 2015 results. XIII. Cosmological parameters
• The Structure of Cold Dark Matter Halos
• Theory of Bose-Einstein condensation in trapped gases
• Vortex formation in a stirred Bose-Einstein condensate
• Cold and Fuzzy Dark Matter
• Ultralight scalars as cosmological dark matter
• Too big to fail? The puzzling darkness of massive Milky Way subhaloes
• Extra force in $f(R)$ modified theories of gravity
• The Milky Way's bright satellites as an apparent failure of LCDM
• Asymmetric Dark Matter: Theories, Signatures, and Constraints
• Can dark matter be a Bose-Einstein condensate?
• The non-gravitational interactions of dark matter in colliding galaxy clusters
• The Characterization of the Gamma-Ray Signal from the Central Milky Way: A Compelling Case for Annihilating Dark Matter
• Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results
• Bose-Einstein Condensation of Dark Matter Axions
• Background model systematics for the Fermi GeV excess
• Late time Cosmological Phase Transition and Galactic Halo as Bose-liquid
• Stationary states of a rotating Bose-Einstein condensate: routes to vortex nucleation
• Dark matter maps reveal cosmic scaffolding
• Fluid Dark Matter
• The origin of angular momentum in dark matter halos
• Dark matter production in the early Universe: beyond the thermal WIMP paradigm
• Repulsive Dark Matter
• Simulations of solitonic core mergers in ultra-light axion dark matter cosmologies
• Galaxy Masses
• Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: II. Numerical results
• Galactic Searches for Dark Matter
• Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter
• Bose-Einstein Condensate general relativistic stars
• Dark Matter and Background Light
• Understanding the shape and diversity of dwarf galaxy rotation curves in LCDM
• Contrasting Galaxy Formation from Quantum Wave Dark Matter, $\psi$DM, with $\Lambda$CDM, using Planck and Hubble Data
• Angular Momentum and Vortex Formation in Bose-Einstein-Condensed Cold Dark Matter Haloes
• Evolution of cosmological perturbations in Bose-Einstein condensate dark matter
• Galactic Halos of Fluid Dark Matter
• Late-time Phase transition and the Galactic halo as a Bose Liquid: (II) the Effect of Visible Matter
• Can the galactic rotation curves be explained in brane world models?
• Bose-Einstein condensation of dark matter solves the core/cusp problem
• Constraints on Self-Interacting Dark Matter
• The universal rotation curve of dwarf disk galaxies
• A Grand Rotation Curve and Dark Matter Halo in the Milky Way Galaxy
• The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
• Growth of perturbations in an expanding universe with Bose-Einstein condensate dark matter
• Flat Central Density Profile and Constant DM Surface Density in Galaxies from Scalar Field Dark Matter
• Ultra-Light Dark Matter in Ultra-Faint Dwarf Galaxies
• The virial theorem and the dark matter problem in hybrid metric-Palatini gravity
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• Generalized virial theorem in f(R) gravity
• The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
• Cluster Density Profiles as a Test of Modified Gravity
• A Testable Conspiracy: Simulating Baryonic Effects on Self-Interacting Dark Matter Halos
• Minimum mass of galaxies from BEC or scalar field dark matter
• The virial theorem and the dynamics of clusters of galaxies in the brane world models
• Review of the theoretical and experimental status of dark matter identification with cosmic-ray antideuterons
• The core-cusp problem: a matter of perspective
• Mimicking dark matter in galaxy clusters through a non-minimal gravitational coupling with matter
• Declining rotation curves of galaxies as a test of gravitational theory
• Kinematics of the Outer Stellar Halo
• Dark matter component decaying after recombination: lensing constraints with Planck data
• Gravitational effects of condensate dark matter on compact stellar objects
• Effective Theory of WIMP Dark Matter supplemented by Simplified Models: Singlet-like Majorana fermion case
• Complex scalar field dark matter on galactic scales
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• Power spectrum for the Bose-Einstein condensate dark matter
• MOA-II Galactic Microlensing Constraints: The Inner Milky Way has a Low Dark Matter Fraction and a Near Maximal Disk
• Vortices in Bose-Einstein Condensate Dark Matter
• Are galaxies extending?
• A Review of WIMP Baryogenesis Mechanisms
• Gravitational Waves as a New Probe of Bose-Einstein Condensate Dark Matter
• Relativistic self-gravitating Bose-Einstein condensates and cold baryons with a stiff equation of state
• BEC dark matter, Zeldovich approximation and generalized Burgers equation
• Gravitational collapse of Bose-Einstein condensate dark matter halos
• Rotation curves of rotating galactic BEC dark matter halos
• Evolution and dynamical properties of Bose-Einstein condensate dark matter stars
• Galaxy stability within a self-interacting dark matter halo
• Dark matter density profile and galactic metric in Eddington-inspired Born-Infeld gravity
• Cosmological evolution of finite temperature Bose-Einstein Condensate dark matter
• Stability of BEC galactic dark matter halos
• Galactic cold dark matter as a Bose-Einstein condensate of WISPs
• Vortex Structures in a Rotating BEC Dark Matter Component
• Condensate dark matter stars
• Lack of nuclear clusters in dwarf spheroidal galaxies: implications for massive black holes formation and the cusp/core problem
• Instability of a uniformly collapsing cloud of classical and quantum self-gravitating Brownian particles
• Numerical simulation code for self-gravitating Bose-Einstein condensates
• Boson star at finite temperature
• Bose-Einstein condensate strings
• Thin accretion disks around cold Bose-Einstein Condensate stars
• Constraining condensate dark matter in galaxy clusters
• Generalized virial theorem in Palatini $f(R)$ gravity
• Gravitational, lensing, and stability properties of Bose-Einstein condensate dark matter halos
• Evolution of a dwarf satellite galaxy embedded in a scalar field dark matter halo
• Brane-$f(R)$ gravity and dark matter
• Revisiting the constraints on annihilating dark matter by radio observational data of M31
• Discussion on the energy content of the galactic dark matter Bose-Einstein condensate halo in the Thomas-Fermi approximation
• Constraining annihilating dark matter by radio data of M33
• Constraints on Bose-Einstein-condensed Axion Dark Matter from The HI Nearby Galaxy Survey data
• Observational constraints on spinning, relativistic Bose-Einstein condensate stars
• Cosmological perturbations during the Bose-Einstein condensation of dark matter
• On wave dark matter in spiral and barred galaxies
• Virial mass in DGP brane cosmology
• Analytical Approximation for Newtonian Boson Stars in Four and Five Dimensions -- A Poor Person's Approach to Rotating Boson Stars
• Rotation and Angular Momentum Transfer in Bose-Einstein Condensates Induced by Spiral Dark Solitons
• A new target object for constraining annihilating dark matter

Cited by in corpus (25)

• On the possibility of wormhole formation in the galactic halo due to dark matter Bose-Einstein condensates
• Scalar Dark Matter Clumps with Angular Momentum
• Testing Bose-Einstein Condensate dark matter models with the SPARC galactic rotation curves data
• Impact of kinetic and potential self-interactions on scalar dark matter
• Jeans instability and turbulent gravitational collapse of Bose-Einstein Condensate dark matter halos
• Stable vortex in Bose-Einstein condensate dark matter
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Model-independent constraints on ultra-light dark matter from the SPARC data
• Bose-Einstein condensate dark matter model with three-particle interaction and two-phase structure
• Bose-Einstein Condensate dark matter models in the presence of baryonic matter and random confining potentials
• Revealing turbulent Dark Matter via merging of self-Gravitating condensates
• Slowly rotating Bose-Einstein Condensate confronted with the rotation curves of 12 dwarf galaxies
• Rotating Bose-Einstein Condensate Stars at finite temperature
• Partition Function of the Bose-Einstein Condensed Dark Matter and the Modified Gross-Pitaevskii Equation
• Phases of the Bose-Einstein condensate dark matter model with both two- and three-particle interactions
• Superfluid Rayleigh-Plesset extension of FLRW cosmology
• Vortex Lines in Ultralight Bosonic Dark Matter around Rotating Supermassive Black Holes
• Axionlike Dark Matter Model Involving Two-Phase Structure and Two-Particle Composites (Dimers)
• Collective Excitations of Self-Gravitating Bose-Einstein Condensates: Breathing Mode and Appearance of Anisotropy under Self-Gravity
• New Deformed Heisenberg Algebra from the $\mu$-Deformed Model of Dark Matter
• Torquing the Condensate: Angular Momentum Transport in Bose-Einstein Condensates by Solitonic "Corkscrew"
• The decaying and scattering properties of the $d^{\ast }$(2380) hexaquark Bose Einstein Condensate dark matter
• Macroscopic states in Bose-Einstein condensate dark matter model with axionlike interaction
• Boson dark matter halos with a dominant noncondensed component