AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
arXiv:1801.08144 · doi:10.1093/mnras/sty1224
Abstract
We present a new module of the parallel N-Body code P-GADGET3 for cosmological simulations of light bosonic non-thermal dark matter, often referred as Fuzzy Dark Matter (FDM). The dynamics of the FDM features a highly non-linear Quantum Potential (QP) that suppresses the growth of structures at small scales. Most of the previous attempts of FDM simulations either evolved suppressed initial conditions, completely neglecting the dynamical effects of QP throughout cosmic evolution, or resorted to numerically challenging full-wave solvers. The code provides an interesting alternative, following the FDM evolution without impairing the overall performance. This is done by computing the QP acceleration through the Smoothed Particle Hydrodynamics (SPH) routines, with improved schemes to ensure precise and stable derivatives. As an extension of the P-GADGET3 code, it inherits all the additional physics modules implemented up to date, opening a wide range of possibilities to constrain FDM models and explore its degeneracies with other physical phenomena. Simulations are compared with analytical predictions and results of other codes, validating the QP as a crucial player in structure formation at small scales.
18 pages
References in corpus (12)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- A direct empirical proof of the existence of dark matter
- Ultralight scalars as cosmological dark matter
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- A search for ultra-light axions using precision cosmological data
- Axion dark matter, solitons, and the cusp-core problem
- Ultra-Light Scalar Fields and the Growth of Structure in the Universe
- On the Schrodinger-Poisson--Vlasov-Poisson correspondence
- Thermal conduction in cosmological SPH simulations
- Cosmological particle-in-cell simulations with ultralight axion dark matter
- Non-linear hydrodynamics of axion dark matter: relative velocity effects and "quantum forces"
- Cosmology with the Square Kilometre Array
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- Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal
- Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
- i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
- Scalar field dark matter with a cosh potential, revisited
- Diluted Axion Star Collisions with Neutron Stars
- COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
- Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
- SCALAR: an AMR code to simulate axion-like dark matter models
- Minimum star-forming halo mass in axion cosmology
- Abundance matching for low mass galaxies in the CDM and FDM models
- Implications of multi-axion dark matter on structure formation
- Single and merger soliton dynamics in scalar field dark matter with and without self-interactions
- Spherical collapse of fuzzy dark matter
- Nonlinear cosmological structure with ultralight bosons via modified gravity
- Theory and phenomenology of stressed wave-dark-matter soliton
- Dark Matter Annihilation Feedback in Cosmological Simulations II: The Influence on Gas and Halo Structure
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- Dynamic Zoom Simulations: a fast, adaptive algorithm for simulating lightcones
- Vortices and rotating solitons in ultralight dark matter
- Interference in Fuzzy Dark Matter Filaments: Idealised Models and Statistics
- The Effective Field Theory of Large Scale Structures of a Fuzzy Dark Matter Universe
- Comparison of two different integration methods for the (1+1)-Dimensional Schrödinger-Poisson Equation
- The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
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