Invisible dark matter is one of the greatest mysteries in physics. We know it exists because we see how it pulls on stars: Vera Rubin noticed that galaxies spin too fast, and Fritz Zwicky first spoke of hidden mass. It is believed that dark matter appeared right after the Big Bang, in an era that Georges Lemaître first described. To catch it, scientists used a clever trick. Imagine a dark room with an invisible cat. If you toss ping-pong balls into the room (these are cosmic rays, mostly hydrogen nuclei) then occasionally a ball will hit the cat, producing a soft jingle. That jingle is a neutrino, a ghostly particle that races nearly at the speed of light and barely interacts with anything. Especially many of these "jingles" should come from the center of the Galaxy, where a supermassive black hole slumbers surrounded by dark matter.

Armed with 13 years of data from the ANTARES neutrino telescope installed at the bottom of the Mediterranean Sea, researchers "listened" to the Galactic Ridge. They sorted the neutrino signals by energy, just like spectroscopy splits light into a rainbow, and compared them to what was expected from collisions with dark matter. No clear excess was found, and that's already a result: it allowed them to set a strict upper limit on the interaction strength. This approach is reminiscent of the transit method for finding planets, which catches a tiny dimming of stars, except here we're looking for a spike rather than a dip. Unlike the Hubble Space Telescope, which sees the Universe in familiar light, neutrino telescopes peer through gas and dust, and together with future observations of gravitational waves they could assemble the full picture. Even though quantum correlations underlie the collisions, precise models and years of statistics played the decisive role.