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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/025/01-02/0067-0080

    • Keywords

       

      Cosmology: theory; observations; large scale structures-radiation

    • Abstract

       

      We simulate the distribution of neutral hydrogen (HI) at the redshiftsz = 1.3 and 3.4 using a cosmological N-body simulation along with a prescription for assigning HI masses to the particles. The HI is distributed in clouds whose properties are consistent with those of the damped Lyman-a absorption systems (DLAs) seen in quasar spectra. The clustering properties of these clouds are identical to those of the dark matter. We use this to simulate the redshifted HI emission expected at 610 MHz and 325 MHz, two of the observing bands at the GMRT. These are used to predict the correlations expected between the complex visibilities measured at different baselines and frequencies in radio-interferometric observations with the GMRT. The visibility correlations directly probe the power spectrum of HI fluctuations at the epoch when the HI emission originated, and this holds the possibility of using HI observations to study large-scale structures at highz.

    • Author Affiliations

       

      Somnath Bharadwaj1 Pennathur Sridharan Srikant2 3

      1. Department of Physics and Meteorology and Center for Theoretical Studies, I.I.T., Kharagpur - 721 302, India
      2. Department of Physics and Meteorology, I.I.T., Kharagpur - 721 302, India
      3. Department of Physics, University of Utah, USA
    • Dates

       
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