21cm forest probes on the axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenarios
arXiv:2005.05589 · doi:10.1103/PhysRevD.102.023522
Abstract
We study the future prospects of the 21cm forest observations on the axion-like dark matter when the spontaneous breaking of the global Peccei-Quinn (PQ) symmetry occurs after the inflation. The large isocurvature perturbations of order unity sourced from axion-like particles can result in the enhancement of minihalo formation, and the subsequent hierarchical structure formation can affect the minihalo abundance whose masses can exceed relevant for the 21cm forest observations. We show that the 21cm forest observations are capable of probing the axion-like particle mass in the range eV for the temperature independent axion mass. For the temperature dependent axion mass, the zero temperature axion mass scale for which the 21cm forest measurements can be affected is extended further to as big as of order eV.
arXiv comment11 pages, 6 figures, published in PRD
References in corpus (59)
- A Universal Density Profile from Hierarchical Clustering
- Large scale bias and the peak background split
- Axion Cosmology
- String Axiverse
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Axions In String Theory
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- In the Beginning: The First Sources of Light and the Reionization of the Universe
- New CAST Limit on the Axion-Photon Interaction
- Universe Reheating after Inflation
- 21-cm Tomography of the Intergalactic Medium at High Redshift
- A SQUID-based microwave cavity search for dark-matter axions
- The Formation and Fragmentation of Primordial Molecular Clouds
- Optical and Radio Properties of Extragalactic Sources Observed by the FIRST and SDSS Surveys
- First constraints on fuzzy dark matter from Lyman- forest data and hydrodynamical simulations
- A Photometric Redshift of z ~ 9.4 for GRB 090429B
- Probing the Universe with the Lyman-alpha Forest: I. Hydrodynamics of the Low Density IGM
- Simulations of Pregalactic Structure Formation with Radiative Feedback
- Axion Cosmology Revisited
- X-ray gas density profile of clusters of galaxies from the universal dark matter halo
- On Effective Degrees of Freedom in the Early Universe
- Dark Matter from an ultra-light pseudo-Goldsone-boson
- Early seeds of axion miniclusters
- Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres
- Large-amplitude isothermal fluctuations and high-density dark-matter clumps
- Suppression of H_2 Cooling in the Ultraviolet Background
- The one-dimensional power spectrum from the SDSS DR14 Ly forests
- Axion Dark Matter Detection with CMB Polarization
- HI 21cm absorption beyond the epoch of re-ionization
- The Quest for an Intermediate-Scale Accidental Axion and Further ALPs
- Structure Formation and Microlensing with Axion Miniclusters
- Suppression and Spatial Variation of Early Galaxies and Minihalos
- Cosmic strings from preheating
- The radio telescope search for the resonant conversion of cold dark matter axions from the magnetized astrophysical sources
- The 21 cm Forest: Radio Absorption Spectra as Probes of Minihalos Before Reionization
- Constraining the radio-loud fraction of quasars at z>5.5
- Early structure in LCDM
- Axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenario
- Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal
- Astrophysical Effects of Scalar Dark Matter Miniclusters
- The first blazar observed at z>6
- Gravitational Lensing Signatures of Axion Dark Matter Minihalos in Highly Magnified Stars
- PAPER-64 Constraints On Reionization II: The Temperature Of The z=8.4 Intergalactic Medium
- Axion minicluster power spectrum and mass function
- A powerful radio-loud quasar at the end of cosmic reionization
- Miniclusters in the Axiverse
- Modeling the Counts of Faint Radio Loud Quasars: Constraints on the Supermassive Black Hole Population and Predictions for High Redshift
- Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
- The 21 Centimeter Forest
- The 21 cm Forest as a Probe of the Reionization and the Temperature of the Intergalactic Medium
- The earliest galaxies seen in 21 cm line absorption
- Measuring the X-ray Background in the Reionization Era with First Generation 21 cm Experiments
- A Radio Astronomy Search for Cold Dark Matter Axions
- Constraints on nature of ultra light dark matter particles with 21cm forest
- Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario
- Cosmologically probing ultra-light particle dark matter using 21 cm signals
- CMB probes on the correlated axion isocurvature perturbation
- Axion inflation with cross-correlated axion isocurvature perturbations
Cited by in corpus (12)
- 21 cm Forest Constraints on Primordial Black Holes
- Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
- Deep learning-driven likelihood-free parameter inference for 21-cm forest observations
- Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
- Analyzing the 21cm forest with Wavelet Scattering Transform: Insight into non-Gaussian features of the 21cm forest
- Prospects of a statistical detection of the 21-cm forest and its potential to constrain the thermal state of the neutral IGM during reionization
- Impact of dark matter-baryon relative velocity on the 21cm forest
- Boosting the 21 cm forest signals by the clumpy substructures
- Survival of Gas in Subhalos and Its Impact on the 21 cm Forest Signals: Insights from Hydrodynamic Simulations
- How light can ALP dark matter be?
- Probing power spectrum enhancement at small scales with the SKA
- Efficient neutral-IGM inference from noisy 21-cm forest spectra with latent-space U-Net encoding and XGBoost