The Core-Cusp Problem

Abstract

This paper gives an overview of the attempts to determine the distribution of dark matter in low surface brightness disk and gas-rich dwarf galaxies, both through observations and computer simulations. Observations seem to indicate an approximately constant dark matter density in the inner parts of galaxies, while cosmological computer simulations indicate a steep power-law-like behaviour. This difference has become known as the "core/cusp problem", and remains one of the unsolved problems in small-scale cosmology.

Accepted for "Dwarf Galaxy Cosmology" special issue of Advances in Astrophysics

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• Self-similar solutions for Fuzzy Dark Matter
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• Coherent Self-Interactions of Dark Matter in the Bullet Cluster
• On galaxy rotation curves from a continuum mechanics approach to modified gravity
• Analytic expressions for the dark matter-baryon relations
• Emergence of a stellar cusp by a dark matter cusp in a low-mass compact ultra-faint dwarf galaxy
• A 5deg x 5deg deep HI survey of the M81 group: II. HI distribution and kinematics of IC 2574 and HIJASS J1021+68
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Calibrating galaxy formation effects in galactic tests of fundamental physics
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• On the offset of the DM cusp and the interpretation of the 130 GeV line as a DM signal
• Low Mass Pseudoscalar Dark Matter in an Extended B - L Model
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Properties of self-gravitating quasi-stationary states
• Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation
• Composite self-interacting dark matter and Higgs
• PoPE: A population-based approach to model spatial structure of astronomical systems
• Constraining Ultralight Axions with Galaxy Surveys
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• Self-interacting dark matter constraints in a thick dark disk scenario
• Constraining Dwarf Spheroidal Dark Matter Halos With The Galactic Center Excess
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• Stochastic dark matter: Covariant Brownian motion from Planckian discreteness
• Gravitational Waves from Primordial Black Hole Dark Matter Spikes
• Gravitational wave lensing: probing Fuzzy Dark Matter with LISA
• Nuclear star clusters as probes of dark matter halos: the case of the Sagittarius Dwarf Spheroidal Galaxy
• Hunting for Dark Matter Subhalos in Strong Gravitational Lensing with Neural Networks
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Dark mesons as self-interacting dark matter
• Relativistic structure of a supermassive black hole embedded in the dark matter halo of NGC 4649 (M60)
• Dissipative dark matter explains rotation curves
• Satellites in the Local Group and Other Nearby Groups
• Supermassive black hole in NGC 4649 (M60) with a dark matter halo: Impact on shadow measurements and thermodynamic properties
• KeV scale new fermion from a hidden sector
• Vector-fermion dark matter
• Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A${}^{\star }$
• Kinetic recoupling of dark matter
• Warm dark matter sterile neutrinos in electron capture and beta decay spectra
• Thin-disk models in an Integrable Weyl-Dirac theory
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Constraining dark matter halo profiles with symbolic regression
• Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Using dust to constrain dark matter models
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Lensed fast radio bursts as a probe of time-varying gravitational potential induced by wave dark matter
• Probing black holes via quasinormal modes in a dark energy-induced dark matter
• Construction of fuzzy dark matter halos with arbitrary initial velocities
• Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-Faint Dwarf
• Metamorphosis of dwarf halo density profile under dark matter decays
• Dynamical origin of neutrino masses and dark matter from a new confining sector
• Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
• Testing the sterile neutrino dark matter paradigm with astrophysical observations
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• The density profile of Milky Way dark matter halo constrained from the OGLE microlensing sky map
• The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations
• ngravs: Distinct gravitational interactions in GADGET-2
• Morphology of dark matter haloes beyond triaxiality
• Asymmetric Reheating by Primordial Black Holes
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• Evolving Ultralight Scalars into Non-Linearity with Lagrangian Perturbation Theory
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Gamma rays from dark matter
• Ringdown of a black hole sourced by a Burkert-density effective anisotropic source
• Fundamental fields around compact objects: Massive spin-2 fields, Superradiant instabilities and Stars with dark matter cores
• The dark halo of the Hydra I galaxy cluster: core, cusp, cosmological? Dynamics of NGC 3311 and its globular cluster system
• Fast particle-mesh code for Milgromian dynamics
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Strongly-interacting massive particle and dark photon in the era of intensity frontier
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• Impact of Gravitational Slingshot of Dark Matter on Galactic Halo Profiles
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• The Local Dark Matter Density
• Limits in late time conversion of cold dark matter into dark radiation
• Measuring the boson mass of fuzzy dark matter with stellar proper motions
• Phase transitions, anomalous baryon number violation and electroweak multiplet dark matter
• (1+1)-Dimensional Schrödinger-Poisson equation with contact interaction
• A Dynamical-Photometric Phase Space for Spiral Galaxies: Probing the Local Coupling Between Light and Gravity
• Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems
• Structure Formation with Dark Magnetohydrodynamics
• The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
• Probing late-time annihilations of oscillating asymmetric dark matter via rotation curves of galaxies
• Universal Basic Mass Density inside Dark Matter Halos
• Nonlinear instability and solitons in a self-gravitating fluid
• A simple ghost free and caustic free mimetic scalar field dark matter model
• On the Presence of Angular-Velocity Offsets in Disk Galaxies
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
• Structure-wide dark matter density depletion induced by local degeneracies
• A comprehensive analysis using 9 dark matter halo models on the spiral galaxy NGC 4321
• Can Bars Erode Cuspy Halos ?
• Comparing dark matter and MOND hyphotheses from the distribution function of A, F, early-G stars in the solar neighbourhood
• Distinguishing Dark Matter Cusps from Cores using Globular Clusters
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Constraining D-foam via the 21-cm Line
• Mirror magnetic field and its impact on dark matter distribution in galaxies
• Understanding disk galaxy rotation velocities without dark matter contribution--a physical process for MOND?
• Effect of dark matter halos on the orbital and escape dynamics of barred galaxies
• Hypothesis on the nature and origin of cold dark matter
• Dark Matter Universal Properties in Galaxies
• Boson dark matter halos with a dominant noncondensed component
• Dark Matter Phenomenology: Sterile Neutrino Portal and Gravitational Portal in Extra-Dimensions
• CMB Tensor Anisotropies in f(R) Gravity
• Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
• Modeling Solitonic Cores, Stabilization of Bar, and Suppression of Bar Dissolution in DDO 168 via GPP Formalism: A Detailed Analysis of Bose--Einstein Condensate/Fuzzy Dark Matter Halo Structure and Bar Dynamics in the Dwarf Galaxy DDO 168