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Remote Infrared Absorption Spectroscopy with Undetected Photons

This paper demonstrates the first remote open-path Fourier-transform infrared spectroscopy of atmospheric gases, such as butane and methane, over distances up to 43.4 meters by reconstructing mid-infrared spectra using only near-infrared photon detection via co-propagating photon pairs and a pump laser.

Original authors: Simon Neves, Fériel Armbruster, Jean-Pierre Wolf

Published 2026-07-21
📖 4 min read🧠 Deep dive

Original authors: Simon Neves, Fériel Armbruster, Jean-Pierre Wolf

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

Imagine you are a detective trying to identify a thief who is hiding in a dark, foggy room. To catch them, you usually need a special flashlight that can see through the fog, but these flashlights are expensive, fragile, and need to be kept in a freezer to work. Now, imagine a clever trick where you don't need to shine the special flashlight on the thief at all. Instead, you send out a pair of magical twins: one twin is a "visible" messenger that you can easily see and catch, and the other is an "invisible" explorer that goes into the foggy room to sniff out the thief. Even though you never see the invisible explorer, the messenger twin carries a secret message back to you about what the explorer found. By listening to the messenger, you can reconstruct exactly what happened in the fog, without ever needing that expensive, freezer-bound flashlight. This is the essence of a field called "quantum spectroscopy," where scientists use the spooky connection between pairs of light particles to measure things that are usually too hard to detect. It matters because the air around us is filled with invisible gases—some that warm our planet and some that are dangerous leaks—and being able to spot them from far away, without needing bulky or fragile equipment, could help us clean up our atmosphere and stay safe.

The paper you are reading describes a team of scientists who took this "magical twin" trick and used it to sniff out gases in the real world, over a much longer distance than ever before. They built a new kind of "light machine" that sends these twin particles out into the open air, bounces them off a mirror, and brings them back to a detector. The big breakthrough here is that they managed to send these light twins over a distance of 43.4 meters (about 142 feet) through the outdoor atmosphere and still get a clear reading. Previous attempts at this kind of "remote sensing" were like trying to walk a tightrope; if you tried to make the path longer, the machine would get confused by wind or vibrations and stop working. The authors solved this by designing a setup where the "magic trick" happens in a tiny, stable box, and the light twins travel together in a single beam to the mirror and back. Because they travel together, the wind and shaking of the air don't mess up their connection, making the system incredibly robust.

Using this new, stable setup, the team demonstrated two major successes. First, they simulated a gas leak by releasing n-butane (a gas often found in lighters) into the air along the light beam's path. They were able to detect this release from a distance of 23.3 meters, calculating a concentration of 196 ppm · m ± 74 ppm · m. This proves that the method can spot sudden, dangerous gas leaks from afar. Second, and perhaps even more impressively, they used the system to analyze the natural air itself. By measuring the light after it traveled 21 meters through the outdoor atmosphere, they successfully identified methane (a potent greenhouse gas) and water vapor at their natural levels. They found a methane concentration of 3.0 ppm ± 1.2 ppm and a water vapor concentration of 1.3 × 10⁴ ppm ± 0.2 × 10⁴ ppm.

The paper is very clear about what they did and did not do. They explicitly noted that their spectral noise did not display any visible dependence on the interaction length, meaning the signal quality remained steady even when they changed the distance from 3.0 meters to 43.4 meters. However, they also acknowledged a specific limitation: in certain regions of the spectrum, the water vapor in the air is so thick that it "saturates" the signal, making it hard to see other things in those specific spots. By carefully choosing which parts of the light spectrum to look at, they managed to separate the methane signal from the water vapor noise. This isn't just a computer simulation; they actually built the machine, walked outside, and measured real gases. While they suggest that future versions could be miniaturized to fit in a backpack for field tests against older systems, they stop short of claiming this is a perfect, sub-ppm monitoring tool for background methane just yet. Instead, they present it as a major milestone: the first time this "undetected photon" technique has been used to successfully measure the composition of the open atmosphere, opening the door for a new way to watch over our skies.

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