2004/10/31 by Somnath Bharadwaj, Sanjay K. Pandey, Sanjay Kumar Pandey · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #Neutrino Physics Research #astro-ph
paper · pdf · doi:10.1111/j.1365-2966.2005.08836.x
published as Mon.Not.Roy.Astron.Soc. 358 (2005) 968-976 · 10 pages, 4 figures, Accepted to MNRAS with Minor Changes
arxiv created 2005/02/14 · openalex publication_date 2005/03/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The H i distribution at the epoch of re-ionization (EOR) is largely determined by the sizes and distribution of the ionized regions. In the scenario where the ionized regions have comoving sizes of the order of a few Mpc, the large-scale statistical properties of the H i distribution are dominated by the Poisson noise of the discrete ionized regions and it is highly non-Gaussian. We investigate the possibility of probing re-ionization by studying these non-Gaussian features using future radio-interferometric observations of redshifted 21-cm H i radiation. We develop a formalism relating correlations between the visibilities measured at three different baselines and frequencies to the bispectrum of H i fluctuations. For visibilities at the same frequency, this signal is found to be of the same order as the two visibility correlation, which probes the H i power spectrum. For visibilities at different frequencies, we find that the correlations decay within a frequency difference of ∼ 1 MHz. This implies that it is, in principle, straightforward to extract this H i signal from various contaminants, which are believed to have a continuum spectrum and are expected to be correlated even at large frequency separations.