English

Towards simulating and quantifying the light-cone EoR 21-cm signal

Cosmology and Nongalactic Astrophysics 2017-12-12 v3

Abstract

The light-cone (LC) effect causes the Epoch of Reionization (EoR) 21-cm signal Tb(n^,ν)T_{\rm b} (\hat{\bf{n}}, \nu) to evolve significantly along the line of sight (LoS) direction ν\nu. In the first part of this paper, we present a method to properly incorporate the LC effect in simulations of the EoR 21-cm signal that include peculiar velocities. Subsequently, we discuss how to quantify the second order statistics of the EoR 21-cm signal in the presence of the LC effect. We demonstrate that the 3D power spectrum P(k)P({\bf{k}}) fails to quantify the entire information because it assumes the signal to be ergodic and periodic, whereas the LC effect breaks these conditions along the LoS. Considering a LC simulation centered at redshift 88 where the mean neutral fraction drops from 0.650.65 to 0.350.35 across the box, we find that P(k)P({\bf{k}}) misses out 40%\sim 40 \% of the information at the two ends of the 17.41MHz17.41 \, {\rm MHz} simulation bandwidth. The multi-frequency angular power spectrum (MAPS) C(ν1,ν2){\mathcal C}_{\ell}(\nu_1,\nu_2) quantifies the statistical properties of Tb(n^,ν)T_{\rm b} (\hat{\bf{n}}, \nu) without assuming the signal to be ergodic and periodic along the LoS. We expect this to quantify the entire statistical information of the EoR 21-cm signal. We apply MAPS to our LC simulation and present preliminary results for the EoR 21-cm signal.

Keywords

Cite

@article{arxiv.1706.09449,
  title  = {Towards simulating and quantifying the light-cone EoR 21-cm signal},
  author = {Rajesh Mondal and Somnath Bharadwaj and Kanan K. Datta},
  journal= {arXiv preprint arXiv:1706.09449},
  year   = {2017}
}

Comments

Published in Monthly Notices of the Royal Astronomical Society (MNRAS). Available at http://dx.doi.org/10.1093/mnras/stx2888

R2 v1 2026-06-22T20:32:37.817Z