Abstract:
We examine a type of feature in the primordial scalar power spectrum, namely,
the bump-like feature(s) that arise as a result of burst(s) of particle production during
inflation. The latest CMB observations by Planck 2018 can accommodate the imprints of
such primordial features. In the near future, observations of redshifted 21 cm signal from the
Epoch of Reionization (EoR) can put additional constraints on inflation models by exploiting
the expected tomographic information across a wide range of co-moving wave-numbers. In this
work, we study the potential of upcoming observational data from SKA-Low to constrain the
parameters of the primordial power spectrum with bump-like features. We use simulated mock
data expected from SKA-Low, with uncertainties estimated from different foreground removal
models, and constrain the parameters of primordial features within a Bayesian framework.
We study two scenarios: in the first scenario, where the astrophysical parameters relevant
to the EoR are known, we find that 21 cm power spectra do have the potential to probe
the primordial bump-like features. As the input amplitude of the bump is decreased below
roughly 10% of the amplitude of the primordial power spectrum without the bump, the
uncertainties in the recovered values for both amplitude and location of the bump are foundto increase, and the recovered values of the location of the bump also get increasingly more biased towards higher values. Hence, it becomes harder to constrain these parameters. In the
second scenario, we analyze the achievable constraints on primordial features when two of the
EoR parameters, namely, minimum halo mass and ionizing efficiency, are uncertain. We find
that the effect of the bump on the profile and the amplitude of the 21 cm power spectrum
is distinct from the impact of changing the astrophysical parameters, and hence they may
potentially be distinguished.
