Scalar Field as Dark Matter in the Universe

Abstract

We investigate the hypothesis that the scalar field is the dark matter and the dark energy in the Cosmos, wich comprises about 95% of the matter of the Universe. We show that this hypothesis explains quite well the recent observations on type Ia supernovae.

4 pages REVTeX, 1 eps figure. Minor changes. To appear in Classical and Quantum Gravity

Cited by in corpus (126)

• Quintessence and black holes
• Quintessence arising from exponential potentials
• First constraints on fuzzy dark matter from Lyman-$\alpha$ forest data and hydrodynamical simulations
• Wave Dark Matter
• Simulations of solitonic core mergers in ultra-light axion dark matter cosmologies
• A Further Analysis of a Cosmological Model of Quintessence and Scalar Dark Matter
• Dwarf Galaxy Rotation Curves and the Core Problem of Dark Matter Halos
• Linear and non-linear perturbations in dark energy models
• A new cosmological tracker solution for Quintessence
• Quintessence and Scalar Dark Matter in the Universe
• Galactic Halos of Fluid Dark Matter
• A supermassive boson star at the galactic center?
• Quintessential Haloes around Galaxies
• Ultra-Light Dark Matter in Ultra-Faint Dwarf Galaxies
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• Cosmology with a Variable Chaplygin Gas
• Black hole formation from axion stars
• Inflation, cold dark matter, and the central density problem
• Vector field as a quintessence partner
• Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultra-light boson) scalar field dark matter
• AxioNyx: Simulating Mixed Fuzzy and Cold Dark Matter
• On the mass of ultra-light bosonic dark matter from galactic dynamics
• Oscillatons revisited
• Combining rotation curves and gravitational lensing: How to measure the equation of state of dark matter in the galactic halo
• Scalar Field Dark Matter: Helping or Hurting Small-Scale Problems in Cosmology?
• Axion as a cold dark matter candidate: low-mass case
• Dynamical evolution of fermion-boson stars
• Gravitational waves with dark matter minispikes: the combined effect
• Cosmological parameter inference with Bayesian statistics
• Cosmological perturbations in coherent oscillating scalar field models
• Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints
• Stirred and shaken: dynamical behavior of boson stars and dark matter cores
• Evading Weinberg's no-go theorem to construct mass dimension one fermions: Constructing darkness
• Dynamical formation and stability of fermion-boson stars
• A new approach on the stability analysis in ELKO cosmology
• Slightly Bimetric Gravitation
• Core-Halo Mass Relation in Scalar Field Dark Matter Models and its Consequences for the Formation of Supermassive Black Holes
• The Homogeneous Scalar Field and the Wet Dark Sides of the Universe
• The Cold Dark Matter crisis on galactic and subgalactic scales
• Beyond Schrödinger-Poisson: Nonrelativistic Effective Field Theory for Scalar Dark Matter
• Ultra light bosonic dark matter and cosmic microwave background
• Dynamical $\ell$-boson stars: generic stability and evidence for non-spherical solutions
• First constraints on Fuzzy Dark Matter from the dynamics of stellar streams in the Milky Way
• Numerical evidence for `multi-scalar stars'
• Cosmological structure formation in scalar field dark matter with repulsive self-interaction: The Incredible Shrinking Jeans Mass
• Perturbations of ultralight vector field dark matter
• Dynamical Friction From Ultralight Dark Matter
• Can fermion-boson stars reconcile multi-messenger observations of compact stars?
• Collapse threshold for a cosmological Klein Gordon field
• Modifying PyUltraLight to model scalar dark matter with self-interactions
• Scalar field dark matter in clusters of galaxies
• Galactic rotation curves and brane world models
• Scalar fields properties for flat galactic rotation curves
• How sound are our ultra-light axion approximations?
• Some remarks on the attractor behaviour in ELKO cosmology
• A stabilization mechanism for excited fermion-boson stars
• Is Sextans dwarf galaxy in a scalar field dark matter halo?
• Symmetries leading to inflation
• Vector field and rotational curves in dark galactic halos
• Extreme $\ell$-boson stars
• On the Possibility that Ultra-Light Boson halos host and form Super-massive Black Holes
• Stability analysis and constraints on interacting viscous cosmology
• Gravitational lensing by wave dark matter halos
• Self-interactions of ULDM to the rescue?
• Supergravity in Two Spacetime Dimensions
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
• Small scale structures in coupled scalar field dark matter
• European Spallation Source as a searching tool for an ultralight scalar field
• Scalar Field Dark Matter
• Braneworld Model of Dark Matter: Structure Formation
• Non-relativistic approach for cosmological Scalar Field Dark Matter
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Cosmological constraints on unifying Dark Fluid models
• Multi-fluid cosmology in Einstein gravity: analytical solutions
• Description of the evolution of inhomogeneities on a Dark Matter halo with the Vlasov equation
• Interacting Scalar fields: Dark matter and early dark energy
• Complex Scalar Field Reheating and Primordial Black Hole production
• Solving the Cusp-Core Problem with a Novel Scalar Field Dark Matter
• Testing DM halos using rotation curves and lensing: A warning on the determination of the halo mass
• Rotating 5D-Kaluza-Klein Space-Times from Invariant Transformations
• ULDM self-interactions, tidal effects and tunnelling out of satellite galaxies
• Energy Balance of a Bose Gas in Curved Spacetime
• Phenomemology of a Realistic Accelerating Universe Using Tracker Fields
• A new proposal for Galactic dark matter: Effect of f(T) gravity
• Isotropisation of Bianchi class A models with a minimally coupled scalar field and a perfect fluid
• Solitons and halos for self-interacting scalar dark matter
• Self-interacting scalar field distributions around Schwarzschild black holes
• Consequences for the Scalar Field Dark Matter model from The McGaugh Observed-Baryon Acceleration Correlation
• Bianchi type IX asymptotical behaviours with a massive scalar field: chaos strikes back
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• Ultrarelativistic Bose-Einstein Gas on Lorentz Symmetry Violation
• Single and merger soliton dynamics in scalar field dark matter with and without self-interactions
• Can Dark Matter be a Scalar Field?
• Response to an External Magnetic Field of the Decay Rate of a Neutral Scalar Field into a Charged Fermion Pair
• Solving the Schrodinger Poisson System using the coordinate Adaptive Moving Mesh method
• Evolution of perturbation and power spectrum in a two-component ultralight axionic universe
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Long-wavelength non-linear perturbations of a complex scalar field
• Gravitational atoms beyond the test field limit: The case of Sgr A* and ultralight dark matter
• A Universal SFDM Halo Mass for the Andromeda and Milky Way's dSphs?
• Nonlinear cosmological structure with ultralight bosons via modified gravity
• On particle scattering in Gross-Pitaevskii theory and implications for dark matter halos
• Back reaction of a long range force on a Friedmann-Robertson-Walker background
• Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential
• Dynamical friction in rotating ultralight dark matter galactic cores
• Analytic Solutions of Scalar Field Cosmology, Mathematical Structures for Early Inflation and Late Time Accelerated Expansion
• 3D Vortices and rotating solitons in ultralight dark matter
• Bifurcations in Bosonic Stars: chains and rings from spherical solutions
• Scalar Field Dark Matter: Impact of Supernovae-driven blowouts on the soliton structure of low mass dark matter halos
• Bose-Einstein Condensate Dark Matter That Involves Composites
• Could primordial galactic Magnetic Fields be generated by Charged Ultra-Light Boson Dark Matter?
• From Dark Radiation to Dark Energy: Unified Cosmological Evolution in K-essence Models
• Scaling relations, dynamical heating and tidal disruption in spin $s$ ultralight dark matter models
• On Dark Matter As A Geometric Effect in the Galactic Halo
• Leptons and other forces of Nature
• Fluids in cosmology
• Is it possible to separate baryonic from dark matter within the $\Lambda$-CDM formalism?
• Challenging theories of gravitation: dark matter, compact objects and gravitational waves
• To observe, or not to observe, quantum-coherent dark matter in the Milky Way, that is a question
• Slowly Rotating Boson Stars
• UltraDark.jl: A Julia package for simulation of cosmological scalar fields
• Self-interacting scalar field in (2+1) dimensions Einstein gravity with torsion
• Core-halo scaling relations in self-interacting scalar field dark matter
• Rotation curves with the multistate Scalar Field Dark Matter model
• Ultralight bosonic dark matter in white dwarfs and potential observational consequences