Physicists have coaxed the most famous glow of a black hole out of a strand of optical fiber. For the first time, they watched that light react back on the simulated black hole that produced it. The result gives researchers a rare, hands-on look at Hawking radiation, the faint thermal emission that Stephen Hawking predicted should leak out of black holes. It offers a first clue about the tiny push that could, in principle, make a real black hole slowly evaporate, the research team said in a new study.
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Subscribe Sekarang →Working with a tabletop experiment in optical fibers, the international team detected both the radiation and its long-sought back reaction. This is the way the radiation feeds energy back and reshapes the object that created it. According to the new study, published July 1 in the journal Nature, the light behaved exactly as Hawking predicted it should. It behaved like the glow of a warm object, with a definite temperature and a spectrum that fades away steadily toward higher frequencies. It did so even in a regime where the usual textbook description of a black hole should break down.
Hawking radiation is famous because it sits at the crossroads of the biggest ideas in physics. "Jacob Bekenstein predicted that black holes have an entropy and a temperature, and Hawking calculated the thermal radiation of the black hole," study co-author Ulf Leonhardt, a physicist at the Weizmann Institute of Science in Israel, said. "In Hawking-Bekenstein radiation, quantum physics, general relativity and thermodynamics come together — subjects that are normally in conflict with each other."
The conflict runs deep. General relativity pictures space and time as smooth and continuous, while quantum mechanics describes a world of discrete, unpredictable jumps. No one has managed to fully reconcile the two. That combination is exactly what makes Hawking radiation so hard to study. Astronomers have never seen Hawking radiation from a real black hole and probably never will, as the glow is far too faint to pick out across the cosmos. So physicists have turned to laboratory stand-ins that obey the same equations, building black hole analogues out of flowing water, ultracold atoms and, as in this study, light.
The trick behind every black hole analogue is a moving medium. "Imagine a swimmer in the sea with a current faster than he can swim," Leonhardt explained. "He is swept away. This is what happens beyond the horizon, and this is why normally nothing can escape the black hole." A black hole's event horizon is the boundary where that current, space itself in real life, starts moving faster than anything can travel. To recreate it, the team needed a material that appears to rush along at the speed of light. Their solution was elegant: use light to make the material.
In practice, the researchers fired an intense, ultrashort pump pulse into a thin photonic-crystal fiber, which is a strand of glass threaded with a pattern of tiny air channels running along its length. This design lets researchers fine-tune how light moves through it. As it traveled, the pulse slightly changed how the glass bent light, creating a moving speed bump that raced along with it. A second, much weaker probe pulse then ran into this moving front. Where the probe could no longer keep up, an artificial horizon formed, and the black hole analogue was born.
The payoff came in the ultraviolet. According to theory, Hawking radiation is created in pairs. One partner escapes, while the other, carrying negative energy, is the mirror image that would fall into a real black hole. In the fiber, that partner showed up as ultraviolet light. "We counted photons in the ultraviolet that correspond to the Hawking partners beyond the horizon," Leonhardt explained. "They have a wavelength around 233 nanometers. This was our signal."
Just as important as seeing the glow was understanding how it was made. For years, researchers assumed the fiber built up its Hawking radiation through a cascade, which is a chain of separate steps in which the light is converted first into one intermediate form and then another. The team found that, instead, a single, direct interaction does the job, with the pump and probe light producing the Hawking pair in one clean step. It is a much simpler picture that the researchers said may carry over to other analogues and perhaps even to real black holes.
Because energy has to come from somewhere, making Hawking radiation should nudge the source that created it. For a real black hole, that nudge is how it loses mass and, over unimaginable timescales, evaporates entirely. No experiment had ever captured that recoil. Here, the team saw it. Producing the radiation shifted a small fraction of the pump pulse's own light to a slightly different color, leaving a telltale lopsided pattern in the spectrum. That asymmetry is the fingerprint of the back reaction, the black hole analogue quietly paying the energetic price for its own glow.