Axion Miniclusters Made Easy
arXiv:2006.08637 · doi:10.1103/PhysRevD.103.083525
Abstract
We use a modified version of the Peak Patch excursion set formalism to compute the mass and size distribution of QCD axion miniclusters from a fully non-Gaussian initial density field obtained from numerical simulations of axion string decay. We find strong agreement with N-Body simulations at a significantly lower computational cost. We employ a spherical collapse model and provide fitting functions for the modified barrier in the radiation era. The halo mass function at has a power-law distribution for masses within the range , with all masses scaling as . We construct merger trees to estimate the collapse redshift and concentration mass relation, , which is well described using analytical results from the initial power spectrum and linear growth. Using the calibrated analytic results to extrapolate to , our method predicts a mean concentration . The low computational cost of our method makes future investigation of the statistics of rare, dense miniclusters easy to achieve.
References in corpus (13)
- The NumPy array: a structure for efficient numerical computation
- Discovering the QCD Axion with Black Holes and Gravitational Waves
- Dielectric Haloscopes: A New Way to Detect Axion Dark Matter
- Physics potential of the International Axion Observatory (IAXO)
- The dark-matter axion mass
- Axion cosmology with long-lived domain walls
- Improved estimation of radiated axions from cosmological axionic strings
- Fast Radio Bursts and Axion Miniclusters
- Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres
- Detectability of Axion Dark Matter with Phonon Polaritons and Magnons
- Axion minicluster power spectrum and mass function
- Axion astronomy with microwave cavity experiments
- Destruction of axion miniclusters in the Galaxy
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- Probing Small-Scale Power Spectra with Pulsar Timing Arrays
- Transient Radio Signatures from Neutron Star Encounters with QCD Axion Miniclusters
- Stellar Disruption of Axion Miniclusters in the Milky Way
- Simulations of axion-like particles in the post-inflationary scenario
- Structure of Axion Miniclusters
- Axion minivoids and implications for direct detection
- ALP Dark Matter Mini-Clusters from Kinetic Fragmentation
- Detecting Dark Matter Substructures on Small Scales with Fast Radio Bursts
- Post-inflationary axions: a minimal target for axion haloscopes
- ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
- QCD Axion Kinetic Misalignment without Prejudice
- Axions in Andromeda: Searching for Minicluster -- Neutron Star Encounters with the Green Bank Telescope
- Astrophysical Searches and Constraints on Ultralight Bosonic Dark Matter
- On the Galactic radio signal from stimulated decay of axion dark matter
- Evidence for axion miniclusters with an increased central density
- A self-consistent wave description of axion miniclusters and their survival in the galaxy
- Self-similar kinetics for gravitational Bose-Einstein condensation