9–13 Sept 2026
Tsung-Dao Lee Institute
Asia/Shanghai timezone

Dark Acoustic Oscillations as a Future detector for DM–Proton Scattering, Twin Baryons, and Neutrino Portals

12 Sept 2026, 09:00
30m
Tsung-Dao Lee Institute/S5F-S500 - Lecture Room (Tsung-Dao Lee Institute)

Tsung-Dao Lee Institute/S5F-S500 - Lecture Room

Tsung-Dao Lee Institute

Tsung-Dao Lee Institute, 1 Lisuo Road, Pudong New Area, Shanghai,201210

Speaker

Yue-Lin Sming Tsai (Purple Mountain Observatory)

Description

Dark Acoustic Oscillations (DAO) are characteristic wiggles and cutoffs in the matter power spectrum that probe non-gravitational dark matter (DM) interactions. We synthesize four recent analyses. Inelastic self-scattering in a two-component dark sector generates DAO via exothermic conversion and suppresses small-scale structure. Elastic DM–proton scattering imprints DAO on weak lensing. Our DES Year 3 analysis sets upper limits five times stronger than Planck CMB constraints. In the Mirror Twin Higgs framework, DAO from twin-sector couplings simultaneously alleviate the Hubble and S8​ tensions. DM–neutrino interactions yield a nearly 3σ preference when combining early Universe data with DES Y3 cosmic shear, resolving the S8 discrepancy. Critically, China Space Station Telescope (CSST) forecasts project an order-of-magnitude improvement on DM–proton scattering limits and 10% precision on twin baryon abundance. CSST will use these four DAO signals to test dark matter interactions beyond the standard cosmological model.

Presentation materials