Unveiling the microscopic nature of dark matter is one of the biggest challenges in modern physics, and a key research goal at the Tsung-Dao Lee Institute. One important approach is indirect detection, which searches for astrophysical signals from dark matter annihilation or decay into Standard Model particles such as photons or neutrinos.

Near supermassive black holes, extreme gravity can concentrate dark matter into dense “spikes,” with energy densities orders of magnitude higher than those in the solar neighborhood. This greatly enhances annihilation rates, making these regions uniquely promising for observation.

The EHT’s images of the supermassive black hole M87* reveal a dark “shadow” encircled by a bright photon ring. The study shows that the faintest region of this shadow, the “inner shadow,” shaped by light bending near the horizon, is especially sensitive to radiation from dark matter annihilation. Unlike ordinary plasma, typically expelled by jets, dark matter annihilation continuously injects electron–positron pairs, which radiate synchrotron light and illuminate this otherwise dark zone, as shown in the right panel of Fig. 1.

Figure 1: Simulated images of the supermassive black hole M87*: left panel shows radiation from astrophysical plasma; right panel illustrates potential emission from dark matter annihilation.

To ensure robust constraints, the authors developed the most advanced framework to date for modeling electron–positron propagation in the strong gravity and magnetic fields near black holes, grounded in general relativistic magnetohydrodynamic simulations calibrated to current EHT data. Their results rule out wide ranges of previously unexplored dark matter models and establish black hole imaging as a new frontier for fundamental physics. Looking ahead, upgrades to the EHT—particularly improvements in dynamic range—will sharpen sensitivity by probing even darker shadow regions.