Detectability of the 21 cm-CMB cross-correlation from the EoR
arXiv:0908.1632 · doi:10.1111/j.1365-2966.2009.16078.x
Abstract
The 21-cm line fluctuations and the cosmic microwave background (CMB) are powerful probes of the epoch of reionisation of the universe. We study the potential of the cross-correlation between 21-cm line fluctuations and CMB anisotropy to obtain further constraints on the reionisation history. We compute analytically the 21-cm cross-correlation with the CMB temperature anisotropy and polarisation, and we calculate the signal-to-noise (SN) ratio for its detection with Planck together with LOFAR, MWA and SKA. We find, on the one hand, that the 21-cm cross-correlation signal with CMB polarisation from the instant reionisation can be detected with an SN ratio of for LOFAR and for SKA. On the other hand, we confirm that the detection of the 21-cm cross-correlation with CMB polarisation is practically infeasible.
12 figures
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Cited by in corpus (10)
- The Epoch of Reionization
- The Kinetic Sunyaev-Zel'dovich Effect from Reionization: Simulated Full Sky Maps at Arcminute Resolution
- Background reionization history from omniscopes
- Probing patchy reionization through tau-21cm correlation statistics
- Reconstructing large scales at cosmic dawn
- Exploring the cosmic dawn and epoch of reionization with 21cm line
- Constraining primordial non-Gaussianity with CMB-21cm cross-correlations?
- Detectability of the -21cm cross-correlation: a tomographic probe of patchy reionization
- Study of systematics effects on the Cross Power Spectrum of 21 cm Line and Cosmic Microwave Background using Murchison Widefield Array Data
- Reionization and CMB non-Gaussianity