Speaker
Sambit Kumar Giri
(Stockholm University)
Description
The low-frequency component of the Square Kilometre Array (SKA) will be able to observe the 21-cm signal produced by the neutral hydrogen in the intergalactic medium (IGM) during the epoch of reionization (EoR). Using this signal, we can study the evolution of large scale structures during the Reionization epochs. In this talk, I will present a fast framework to model the signal that is vital for interpreting the upcoming SKA data. I will also show a forecast study highlighting the capability of the expected 21-cm signal from SKA in constraining the cosmological parameters.
Primary author
Sambit Kumar Giri
(Stockholm University)
