paper

The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization

arXiv:2605.18939

Abstract

Patchy reionization couples the ionized-bubble morphology to the underlying density field, making the CMB Thomson optical depth sensitive to both the global ionization history and anisotropic fluctuations on the sky. Using the large-volume radiation-hydrodynamical Lumina simulation, we compute in two ways: (i) from global volume- and mass-weighted ionization histories, and (ii) from explicit line-of-sight integrations through on-the-fly light cones. We find that the sightline-averaged optical depth in the light cone, , exceeds the value inferred from a global volume-weighted history, , by . This enhancement is largely captured by the global mass-weighted prediction, , indicating that precision comparisons to CMB optical-depth constraints should use mass-weighted electron fractions or explicit light-cone integration rather than volume-weighted ionized fractions alone. The excess optical depth accumulates primarily near , where the combination of high physical density and strong ionization-field patchiness is greatest. The resulting field is non-Gaussian and exhibits sightline-to-sightline scatter, with fluctuations tracing rare early-ionized overdensities and large-scale structure. Coarse-graining experiments show that smoothing the ionization field on scales suppresses the density-ionization correlation and biases low relative to the resolved calculation. Finally, angular power spectra and real-space correlation functions decomposed into HII, HeII, and HeIII auto- and cross-contributions reveal scale-dependent departures from simple hydrogen-helium co-tracing and evolving characteristic scales with redshift.

20 pages, 20 figures. Submitted to OJA. Please visit https://lumina-simulation.com/ for more details

The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization · wovepaper