Probing the Dark Ages with the Square Kilometer Array

Details Probing the Dark Ages with the Square Kilometer Array Probing the Dark Ages with the Square Kilometer Array

2004-09-13

arxiv.org/abs/astro-ph/0409312v2

New Astron.Rev. 48 (2004) 1029-1038

Astronomy and Astrophysics

Astrophysics

espcrc2.sty, 12 pages. to appear in: "Science with the Square Kilometer Array," New Astronomy Reviews, eds. C. Carilli, S. Raw

Scientific paper

10.1016/j.newar.2004.09.046

The epoch of reionization (EoR) sets a fundamental benchmark in cosmic structure formation, corresponding to the formation of the first luminous objects that act to ionize the neutral intergalactic medium (IGM). Recent observations at near-IR and radio wavelengths imply that we are finally probing into this key epoch of galaxy formation at $z \ge 6$. The Square Kilometer Array (SKA) will provide critical insight into the EoR in a number of ways. First, the ability of the SKA to image the neutral IGM in 21cm emission is a truly unique probe of the process of reionization, and is recognized as the next necessary and fundamental step in our study of the evolution of large scale structure and cosmic reionization. Second, study of HI 21cm absorption toward the first radio loud objects probes small to intermediate scale structure in the neutral 'cosmic web', as well as HI in the first collapsed structures (proto-disks and mini-halos). And third, the incomparable sensitivity of the SKA allows for the study of the molecular gas, dust, and star formation activity in the first galaxies, as well as the radio continuum emission from the first accreting massive black holes. Such objects will be obscured at optical wavelengths due to absorption by the neutral IGM.

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