- Open Access
Forecasting the Ly- forest CMB lensing bispectrum from ACT, SO, S4, and DESI
Phys. Rev. D 112, 063528 – Published 16 September, 2025
DOI: https://doi.org/10.1103/9x9x-pqqm
Abstract
We forecast the sensitivity of future correlations between cosmic microwave background (CMB) lensing and the Lyman- forest power spectrum. This squeezed-limit bispectrum probes the connection between the Lyman- transmission and the underlying large-scale matter density field. We recover the measured signal-to-noise (SNR) ratio obtained with , and forecast a SNR of 10.3,14.8 and 20.2 for DESI combined with ACT, SO, and CMB-S4, respectively. For DESI and SO/CMB-S4, the correlation should be detectable at in 5 redshift bins, useful for distinguishing our signal from several contaminants. Indeed, our forecast is affected by large theoretical uncertainties in the current modeling of the signal and its contaminants, such as continuum misestimation bias or damped-Lyman- absorbers. Quantifying these more accurately will be crucial to enable a reliable cosmological interpretation of this observable in future measurements. We attempt to enumerate the features required in future Lyman- forest simulations required to do so.
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