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    • Fulltext

       

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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/044/0010

    • Keywords

       

      Galaxies: high-redshift; intergalactic medium; cosmology: theory.

    • Abstract

       

      In this review article, we briefly outline our current understanding of the physics associated with the HI 21-cm signal from cosmic dawn. We discuss different phases of cosmic dawn as the ambient gas and the background radiations evolve with the redshift. We address the consequences of several possible heating sources and radiation background on the global 21-cm signal. We further review our present perspective of other important aspects of the HI 21-cm signal, such as power spectrum and imaging. Finally, we highlight thefuture key measurements of the Square Kilometre Array and other ongoing/upcoming experiments that will enlighten our understanding of the early Universe.

    • Author Affiliations

       

      ANKITA BERA1 RAGHUNATH GHARA2 ATRIDEB CHATTERJEE3 KANAN K. DATTA4 SAUMYADIP SAMUI1 5

      1. Department of Physics, Presidency University, 86/1 College Street, Kolkata 700073, India.
      2. ARCO (Astrophysics Research Center), Department of Natural Sciences, The Open University of Israel, 1 University Road, PO Box 808, 4353701 Ra’anana, Israel.
      3. National Centre for Radio Astrophysics, TIFR, Post Bag 3, Ganeshkhind, Pune 411007, India.
      4. Department of Physics, Jadavpur University, 188, Raja S.C. Mallick Rd, Kolkata 700032, India.
      5. School of Astrophysics, Presidency University, 86/1 College Street, Kolkata 700073, India.

    • Dates

       
      Published
      4 February 2023
      Manuscript received
      17 March 2022
      Accepted
      27 September 2022
      Final version published online
      4 February 2023

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

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