Constraining isocurvature perturbations with the 21cm emission from minihaloes
arXiv:1311.2585 · doi:10.1093/mnras/stu059
Abstract
We investigate the effects of isocurvature perturbations on the 21cm radiation from minihaloes (MHs) at high redshifts and examine constraints on the isocurvature amplitude and power spectrum using the next generation of radio telescopes such as the Square Kilometre Array. We find that there is a realistic prospect of observing the isocurvature imprints in the 21cm emission from MHs, but only if the isocurvature spectral index is close to (i.e., the spectrum is blue). When the isocurvature fraction increases beyond of the adiabatic component, we observe an unexpected decline in the 21cm fluctuations from small-mass MHs, which can be explained by the incorporation small MHs into larger haloes. We perform a detailed Fisher-matrix analysis, and conclude that the combination of future CMB and 21cm experiments (such as CMBPol and the Fast-Fourier-Transform Telescope) is ideal in constraining the isocurvature parameters, but will stop short of distinguishing between CDM and baryon types of isocurvature perturbations, unless the isocurvature fraction is large and the spectrum is blue.
14 pages, 9 figures, 1 table, accepted for MNRAS
References in corpus (12)
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating
- Non-Gaussianity, Spectral Index and Tensor Modes in Mixed Inflaton and Curvaton Models
- The 21cm angular-power spectrum from the dark ages
- The Fast Fourier Transform Telescope
- Axion isocurvature fluctuations with extremely blue spectrum
- Isocurvature, non-gaussianity and the curvaton model
- Forecasted 21 cm constraints on compensated isocurvature perturbations
- Late Gas accretion onto Primordial Minihalos: a Model for Leo T, Dark Galaxies and Extragalactic High-Velocity Clouds
- Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
- Is the Concentration of Dark Matter Halos at Virialization Universal ?
- Primordial Non-Gaussianity in Models with Dark Matter Isocurvature Fluctuations
Cited by in corpus (13)
- The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
- Small-scale structure and 21cm fluctuations by primordial black holes
- Constraining warm dark matter with 21 cm line fluctuations due to minihalos
- Baryon isocurvature constraints on the primordial hypermagnetic fields
- Cosmological signatures of tilted isocurvature perturbations: reionization and 21cm fluctuations
- 21 cm Angular Power Spectrum from Minihalos as a Probe of Primordial Spectral Runnings
- Distribution of primordial black holes and 21cm signature
- Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization
- A Bump in the Blue Axion Isocurvature Spectrum
- Large Blue Spectral Isocurvature Spectral Index Signals Time-Dependent Mass
- Probing axion dark matter with 21cm fluctuations from minihalos
- Probing isocurvature perturbations with 21-cm global signal in the light of HERA result
- An Analytic Treatment of Underdamped Axionic Blue Isocurvature Perturbations