Status of the $S_8$ Tension: A 2026 Review of Probe Discrepancies
Ioannis Pantos, Leandros Perivolaropoulos

TL;DR
This review analyzes the ongoing $S_8$ tension between early and late-universe measurements, using a new combined CMB framework and compiling recent survey results to assess systematic effects and potential new physics.
Contribution
It introduces a unified 2026 baseline analysis of $S_8$ combining multiple CMB datasets and compares recent survey results to evaluate the tension and its possible origins.
Findings
Combined CMB analysis yields $S_8=0.836^{+0.012}_{-0.013}$ with reduced uncertainties.
DES Year 6 results show a $2.4$--$2.7\sigma$ tension in $S_8$, while KiDS results are consistent within $<1\sigma$.
Survey-specific systematics likely contribute to discrepancies, but new physics cannot be ruled out.
Abstract
The parameter quantifies the amplitude of matter density fluctuations. A persistent discrepancy exists between early-universe CMB observations and late-universe probes. This review assesses the `` tension'' against a new 2026 baseline: a unified ``Combined CMB'' framework incorporating Planck, ACT DR6, and SPT-3G. This combined analysis yields , providing a higher central value and reduced uncertainties compared to Planck alone. Compiling measurements from 2019--2026, we reveal a striking bifurcation: DES Year 6 results exhibit a statistically significant tension of -- in \citep{DESY6}, whereas KiDS Legacy results demonstrate statistical consistency at \citep{Wright2025}. We examine systematic origins of this dichotomy, including photometric redshift calibration,…
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