One of the common descriptions of black holes is that their gravitational pull is so strong, not even light can escape it. Stephen Hawking is famous for (among other things) showing that this isn’t actually true. The Hawking radiation that bears his name allows matter to escape from the grip of a black hole. In fact, Hawking’s work suggests that an isolated black hole would slowly evaporate away and cease to exist.

But his work remains entirely theoretical. Hawking radiation is expected to be so diffuse that we could only detect it if we could somehow find or create a black hole isolated from all other matter. But Jeff Steinhauer of Israel’s Technion has been on a sometimes single-handed quest to develop a system that can accurately model a black hole’s behavior. And, in a recent paper in Nature Physics, Dr. Steinhauer describes how his model system generates what appears to be Hawking radiation.

Searching for the horizon

A feature called the event horizon plays a central role in both Hawking radiation and the new model system. At a real black hole, the space-time outside the event horizon may be distorted by the intense gravity, but the distortion is relatively limited. Inside the event horizon, however, space-time is stretched at a rate that’s faster than the speed of light. Photons can’t escape because the space-time they occupy is getting stretched away from the event horizon faster than the photon can move.