On the Detectability of the Cosmic Dark Ages: 21-cm Lines from Minihalos

Details On the Detectability of the Cosmic Dark Ages: 21-cm Lines from Minihalos On the Detectability of the Cosmic Dark Ages: 21-cm Lines from Minihalos

2003-02-17

arxiv.org/abs/astro-ph/0302335v1

AIP Conf.Proc. 666 (2003) 85-88

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, to appear in The Emergence of Cosmic Structure, the 13th Annual October Astrophysics Conference in Marylan

Scientific paper

10.1063/1.1581774

In the standard Cold Dark Matter (CDM) theory of structure formation, virialized minihalos (with T_vir = 10,000 K or less) form in abundance at high redshift (z > 6), during the cosmic "dark ages." The hydrogen in these minihalos, the first nonlinear baryonic structures to form in the universe, is mostly neutral and sufficiently hot and dense to emit strongly at the 21-cm line. We calculate the emission from individual minihalos and the radiation background contributed by their combined effect. Minihalos create a "21-cm forest" of emission lines. We predict that the angular fluctuations in this 21-cm background should be detectable with the planned LOFAR and SKA radio arrays, thus providing a direct probe of structure formation during the "dark ages." Such a detection will serve to confirm the basic CDM paradigm while constraining the background cosmology parameters, the shape of the power-spectrum of primordial density fluctuations, the onset and duration of the reionization epoch, and the conditions which led to the first stars and quasars. We present results here for the currently-favored, flat LCDM model, for different tilts of the primordial power spectrum. These minihalos will also cause a "21-cm forest" of absorption lines, as well, in the spectrum of radio continuum sources at high redshift, if the latter came into existence before the end of reionization.

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