Towards simulating and quantifying the light-cone EoR 21-cm signal
Abstract
The light-cone (LC) effect causes the Epoch of Reionization (EoR) 21-cm signal T_b (\hat{n}, ν ) to evolve significantly along the line-of-sight (LoS) direction ν. 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 includes 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) 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 centred at redshift 8 where the mean neutral fraction drops from 0.65 to 0.35 across the box, we find that P(k) misses out ∼ 40 per cent of the information at the two ends of the 17.41 MHz simulation bandwidth. The multifrequency angular power spectrum (MAPS) C_{ℓ}(ν_1,ν_2) quantifies the statistical properties of T_b (\hat{n}, ν ) 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.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- February 2018
- DOI:
- 10.1093/mnras/stx2888
- arXiv:
- arXiv:1706.09449
- Bibcode:
- 2018MNRAS.474.1390M
- Keywords:
-
- methods: statistical;
- dark ages;
- reionization;
- first stars;
- diffuse radiation;
- large-scale structure of Universe;
- cosmology: observations;
- cosmology: theory;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- Published in Monthly Notices of the Royal Astronomical Society (MNRAS). Available at http://dx.doi.org/10.1093/mnras/stx2888