English

Measuring patchy reionisation with kSZ$^2$-21 cm correlations

Cosmology and Nongalactic Astrophysics 2018-03-21 v1

Abstract

We study cross-correlations of the kinetic Sunyaev-Zel'dovich effect (kSZ) and 21 cm signals during the epoch of reionisation (EoR) to measure the effects of patchy reionisation. Since the kSZ effect is proportional to the line-of-sight velocity, the kSZ-21 cm cross correlation suffers from cancellation at small angular scales. We thus focus on the correlation between the kSZ-squared field (kSZ2^2) and 21 cm signals. When the global ionisation fraction is low (xe0.7x_e\lesssim 0.7), the kSZ2^2 fluctuation is dominated by rare ionised bubbles which leads to an anti-correlation with the 21 cm signal. When 0.8xe<10.8\lesssim x_e<1, the correlation is dominated by small pockets of neutral regions, leading to a positive correlation. However, at very high redshifts when xe<0.15x_e<0.15, the spin temperature fluctuations change the sign of the correlation from negative to positive, as weakly ionised regions can have strong 21 cm signals in this case. To extract this correlation, we find that Wiener filtering is effective in removing large signals from the primary CMB anisotropy. The expected signal-to-noise ratios for a \sim10-hour integration of upcoming Square Kilometer Array data cross-correlated with maps from the current generation of CMB observatories with 3.4~μ\muK arcmin noise and 1.7~arcmin beam over 100~deg2^2 are 51, 60, and 37 for xe=0.2x_e=0.2, 0.5, and 0.9, respectively.

Keywords

Cite

@article{arxiv.1712.05305,
  title  = {Measuring patchy reionisation with kSZ$^2$-21 cm correlations},
  author = {Q. Ma and K. Helgason and E. Komatsu and B. Ciardi and A. Ferrara},
  journal= {arXiv preprint arXiv:1712.05305},
  year   = {2018}
}

Comments

7pages, 7 figures

R2 v1 2026-06-22T23:18:15.562Z