Investigating the Reionization Epoch through 21\,cm and Line Intensity Mapping Experiments

Abstract

The epoch of reionization (EoR), marking the Universe's transition from a neutral to ionized state, represents a pivotal phase for understanding the formation of the first stars and galaxies. Intensity mapping of atomic and molecular lines, such as $[\mathrm{CII}]$ and CO J-ladder transitions, across a broad redshift range is a powerful tool for investigating star formation history, metallicity, the distribution of gas and dust, and the physical conditions within galaxies. Additionally, 21\,cm line intensity mapping directly probes the neutral hydrogen content in the intergalactic medium, offering a unique window into the timing and morphology of reionization. In this study, we explore the cross-correlation between the 21\,cm signal and multi-line intensity mapping (LIM) to forecast their detectability for next-generation experiments. Our analysis emphasizes the complementary potential of these techniques to constrain parameters such as the minimum mass of ionizing sources and the ionization fraction $x_e$. Cross-correlations with LIM also enable constraints on physical properties like metal enrichment and the relationship between star formation rates and multi-line luminosities. Using mock observations from Square Kilometre Array (SKA)-low 21\,cm and Fred Young Submillimeter Telescope (FYST)-like LIM experiments, we find that the $[\mathrm{CII}]$--21\,cm cross-correlation can constrain reionization history by measuring $x_e$ across multiple redshift bins with significance levels ranging from 9 to 40$σ$. We extend our analysis to CO transitions, showing that the CO(1-0)--21\,cm cross-correlation provides competitive constraints on reionization parameters. The synergies explored here will enable robust constraints on both reionization and LIM parameters, maximizing the scientific return of current and next-generation intensity mapping experiments.