  This work presents an analytical approach for studying the cosmological 21cm
background signal from the Dark Ages (DA) and subsequent Epoch of Reionization
(EoR). We simulate differential observations of a galaxy cluster to demonstrate
how these epochs can be studied with a specific form of the Sunyaev-Zel'dovich
Effect called the SZE-21cm. This work produces simulated maps of the SZE-21cm
and shows that the SZE-21cm can be extracted from future observations with
low-frequency radio interferometers such as the Hydrogen Epoch of Reionization
Array (HERA) and the Square Kilometre Array (SKA). In order to simulate near
realistic scenarios, we look into cosmic variance noise, incorporate and take
into account the effects of foregrounds, thermal noise, and angular resolution
for our simulated observations. We further extend this exploration by averaging
over a sample of galaxy clusters to mitigate the effects of cosmic variance and
instrumental noise. The impact of point source contamination is also studied.
Lastly, we apply this technique to the results of the EDGES collaboration,
which in 2018 reported an absorption feature of the global 21cm background
signal centred at 78 MHz. The challenges to be addressed in order to achieve
the objectives of this work include errors that arise due to cosmic variation,
instrumental noise and point source contamination. Our approach demonstrates
the potential of the SZE-21cm as an indirect probe for the DA and EoR, and we
conclude that the spectral features of the SZE-21cm from our simulated
observations yield results that are close to prior theoretical predictions and
that the SZE-21cm can be used to test the validity of the EDGES detection.
