Will Nonlinear Peculiar Velocity and Inhomogeneous Reionization Spoil 21cm Cosmology from the Epoch of Reionization?
arXiv:1211.2036 · doi:10.1103/PhysRevLett.110.151301
Abstract
The 21cm background from the epoch of reionization is a promising cosmological probe: line-of-sight velocity fluctuations distort redshift, so brightness fluctuations in Fourier space depend upon angle, which linear theory shows can separate cosmological from astrophysical information. Nonlinear fluctuations in ionization, density and velocity change this, however. The validity and accuracy of the separation scheme are tested here for the first time, by detailed reionization simulations. The scheme works reasonably well early in reionization (< 40% ionized), but not late (> 80% ionized).
2 figures, matches published PRL version
References in corpus (1)
Cited by in corpus (7)
- 21 cm signal from cosmic dawn: Imprints of spin temperature fluctuations and peculiar velocities
- The rich complexity of 21-cm fluctuations produced by the first stars
- Nonlinear Bias of Cosmological Halo Formation in the Early Universe
- Redshift-space distortions in simulations of the 21-cm signal from the cosmic dawn
- Reconstructing the nature of the first cosmic sources from the anisotropic 21-cm signal
- Probing early universe through redshifted 21-cm signal: Modelling and observational challenges
- Line of sight anisotropies in the Cosmic Dawn and EoR 21-cm power spectrum