Journal Article

Cross-correlation of the H <span class="smallCaps">i</span> 21-cm signal and Lyα forest: a probe of cosmology

Tapomoy Guha Sarkar, Somnath Bharadwaj, Tirthankar Roy Choudhury and Kanan K. Datta

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 410, issue 2, pages 1130-1134
Published in print January 2011 | ISSN: 0035-8711
Published online December 2010 | e-ISSN: 1365-2966 | DOI:
Cross-correlation of the H i 21-cm signal and Lyα forest: a probe of cosmology

Show Summary Details


Separating the cosmological redshifted 21-cm signal from foregrounds is a major challenge. We present the cross-correlation of the redshifted 21-cm emission from neutral hydrogen (H i) in the post-reionization era with the Lyα forest as a new probe of the large-scale matter distribution in the redshift range z= 2–3 without the problem of foreground contamination. Though the 21-cm and the Lyα forest signals originate from different astrophysical systems, they are both expected to trace the underlying dark matter distribution on large scales. The multifrequency angular cross-correlation power spectrum estimator is found to be unaffected by the discrete quasar sampling, which only affects the noise in the estimate.

We consider a hypothetical redshifted 21-cm observation in a single field of view 1°.3 (FWHM) centred at z= 2.2, where the binned 21-cm angular power spectrum can be measured at a signal-to-noise ratio (S/N) of 3σ or better across the range 500 ≤ℓ≤ 4000. Keeping the parameters of the 21-cm observation fixed, we have estimated the S/N for the cross-correlation signal varying the quasar angular number density n of the Lyα forest survey. Assuming that the spectra have S/N ∼ 5 in pixels of length 44 km s−1, we find that a 5σ detection of the cross-correlation signal is possible at 600 ≤ℓ≤ 2000 with n= 4 deg−2. This value of n is well within the reach of upcoming Lyα forest surveys. The cross-correlation signal will be a new, independent probe of the astrophysics of the diffuse intergalactic medium (IGM), the growth of structure and the expansion history of the Universe.

Keywords: cosmology: theory; diffuse radiation; large-scale structure of Universe

Journal Article.  3981 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.