Missing Beats: Dark Matter Silences Short-Period Cepheids in the Galactic Center

Upcoming near-infrared facilities (e. g. , JWST/NIRCam, ELT/MICADO) will dramatically increase the detectability of galactic center Cepheids despite extreme extinction at optical wavelengths. In this work, we study the impact of dark matter (DM) annihilation on Cepheid stars in the inner parsec of the Milky Way. We show that at densities ρ 10⁵ \, GeV \, cm^-3, blue-loop evolution can be suppressed, preventing the formation of low-mass (3-6 \, M_) short-period (1-6 days) Cepheids. A dearth of such variables could provide indirect evidence for DM heating. Notably, this effect occurs at lower DM densities than required to impact main-sequence stars. Future surveys will thus offer a novel, complementary probe of DM properties in galactic nuclei.