Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
Peng-Ju Wu, Yichao Li, Jing-Fei Zhang, Xin Zhang

TL;DR
This paper forecasts how combining three 21 cm intensity mapping experiments can tightly constrain dark energy parameters and break degeneracies, demonstrating the strategy's effectiveness for future cosmological studies.
Contribution
It introduces a novel joint survey strategy combining FAST, SKA1-MID, and HIRAX for improved dark energy measurements using 21 cm IM data.
Findings
Joint survey tightens cosmological parameter constraints.
Strategy breaks degeneracies in dynamical dark energy models.
Performs well even with lower foreground removal efficiency.
Abstract
The 21 cm intensity mapping (IM) technique provides us with an efficient way to observe the cosmic large-scale structure (LSS). From the LSS data, one can use the baryon acoustic oscillation and redshift space distortion to trace the expansion and growth history of the universe, and thus measure the dark energy parameters. In this paper, we make a forecast for cosmological parameter estimation with the synergy of three 21 cm IM experiments. Specifically, we adopt a novel joint survey strategy, FAST ()+SKA1-MID ()+HIRAX (), to measure dark energy. We simulate the 21 cm IM observations under the assumption of excellent foreground removal. We find that the synergy of three experiments could place quite tight constraints on cosmological parameters. For example, it provides and in…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Superconducting and THz Device Technology · Astronomy and Astrophysical Research
