Prospects for precision cosmology with the 21 cm signal from the dark ages

Author:

Mondal RajeshORCID,Barkana Rennan

Funder

Israel Science Foundation

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Reference32 articles.

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2. Hogan, C. J. & Rees, M. J. Spectral appearance of non-uniform gas at high z. Mon. Not. R. Astron. Soc. 188, 791–798 (1979).

3. Scott, D. & Rees, M. J. The 21-cm line at high redshift: a diagnostic for the origin of large scale structure. Mon. Not. R. Astron. Soc. 247, 510 (1990).

4. Madau, P., Meiksin, A. & Rees, M. J. 21 centimeter tomography of the intergalactic medium at high redshift. Astrophys. J. 475, 429 (1997).

5. Loeb, A. & Zaldarriaga, M. Measuring the small-scale power spectrum of cosmic density fluctuations through 21cm tomography prior to the epoch of structure formation. Phys. Rev. Lett. 92, 211301 (2004).

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