Cosmological forecasts from the baryon acoustic oscillations in 21 cm intensity mapping

In this work, we use a template method to extract the scale associated with the Baryon Acoustic Oscillation (BAO) signal in 21Formula: see textcm neutral hydrogen intensity maps. We then forecast the constraints on the standard deviations of cosmological parameters using a Fisher matrix analysis. In order to test this method, we choose the survey configuration for the BINGO telescope. We then estimate the constraints on the BAO shift parameter Formula: see text, which we extract from the 21Formula: see textcm angular power spectrum (APS). In addition, we translate those results into constraints on the final cosmological parameters. As BAO data alone can only constrain the product of the Hubble constant and the sound horizon Formula: see text, degeneracies between the variables mean that we can’t get useful constraints with BAO data alone. We break these degeneracies by combining the 21Formula: see textcm intensity mapping BAO results with the Cosmic Microwave Background (CMB) covariances obtained by the Planck satellite. In particular, we find that the best forecasts we can get with this combination are on the standard deviations of the Hubble parameter Formula: see text, and the dark energy parameters Formula: see text and Formula: see text. We find Formula: see text (0.8%) in the Formula: see textCDM model. For the wCDM model, we find Formula: see text (2.9%) and Formula: see text (7.5%). In the CPL parameterization, we find Formula: see text (4.4%), Formula: see text (40%), and Formula: see text. Finally, we observe that using the full APS provides stronger constraints than the BAO only, however, it is more susceptible to systematic effects.