Impact of dark matter-baryon relative velocity on the 21cm forest
arXiv:2212.08409 · doi:10.1103/PhysRevD.107.123520
Abstract
We study the effect of the relative velocity between the dark matter (DM) and the baryon on the 21cm forest signals. The DM-baryon relative velocity arises due to their different evolutions before the baryon-photon decoupling epoch and it gives an additional anisotropic pressure that can suppress the perturbation growth. It is intriguing that the scales at which the matter power spectrum is affected by such a streaming velocity turns out to be the scale at which the 21cm forest signal is sensitive to. We demonstrate that the 21cm absorption line abundance can decrease by more than a factor of a few due to the small-scale matter power spectrum suppression caused by the DM-baryon relative velocity.
10pages,9 figures. Accepted in Physical Review D
References in corpus (18)
- The LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release
- The LOFAR Two-metre Sky Survey -- V. Second data release
- The Final SDSS High-Redshift Quasar Sample of 52 Quasars at z>5.7
- HERA Phase I Limits on the Cosmic 21-cm Signal: Constraints on Astrophysics and Cosmology During the Epoch of Reionization
- Supersonic Gas Streams Enhance the Formation of Massive Black Holes in the Early Universe
- Large-scale BAO signatures of the smallest galaxies
- Constraining the radio-loud fraction of quasars at z>5.5
- Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
- Supersonic Relative Velocity between Dark Matter and Baryons: A Review
- The 21 Centimeter Forest
- The earliest galaxies seen in 21 cm line absorption
- Constraints on nature of ultra light dark matter particles with 21cm forest
- 21 cm Forest Constraints on Primordial Black Holes
- The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models
- Exploring the cosmic dawn and epoch of reionization with 21cm line
- 21cm forest probes on the axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenarios
- Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
- Boosting the 21 cm forest signals by the clumpy substructures
Cited by in corpus (4)
- Deep learning-driven likelihood-free parameter inference for 21-cm forest observations
- 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
- Efficient neutral-IGM inference from noisy 21-cm forest spectra with latent-space U-Net encoding and XGBoost