Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping

Abstract

Originally proposed as a cosmological probe of the large-scale structure, line intensity mapping (LIM) also offers a unique window into the astrophysics of galaxy evolution. Adding to the astrophysical explorations of LIM technique that have traditionally focused on small, non-linear scales, we present a novel method to study the global star formation law using forthcoming data from large-scale baryonic acoustic oscillation (BAO) intensity mapping. Using the amplitude of the percent-level but scale-dependent bias induced by baryon fraction fluctuations on BAO scales, we show that combining auto- and cross-correlation power spectra of two (or more) LIM signals allows to probe the star formation law power index $\mathcal{N}$. We examine the prospect for mapping H$\alpha$ and [OIII] lines across all scales, especially where imprints of the baryon fraction deviation exist, with space missions like SPHEREx. We show that although SPHEREx may only marginally probe $\mathcal{N}$ by accessing a modest number of large-scale modes in its 200 deg${}^2$ deep survey, future infrared all-sky surveys reaching a comparable depth with an improved spectral resolution ($R\gtrsim 400$) are likely to constrain $\mathcal{N}$ to a precision of 10$-$30%, sufficient for distinguishing models with varying feedback assumptions, out to $z\sim 4$ using BAO intensity mapping. Leveraging this effect, large, cosmic-variance-limited LIM surveys in the far future can scrutinize the physical connection between galaxy evolution and the large-scale cosmological environment, while performing stringent tests of the standard cosmological model.

arXiv comment9 pages, 4 figures, accepted for publication in ApJL

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Cited by in corpus (6)

• Line-Intensity Mapping: Theory Review
• LIMFAST. II. Line Intensity Mapping as a Probe of High-Redshift Galaxy Formation
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys
• Boosting Line Intensity Map Signal-to-Noise with the Ly-$\alpha$ Forest Cross-Correlation
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping