terahertz spectroscopy

A theater spotlight keeps the actor in its beam no matter where they step. The terahertz radar we are about to describe does the same with a short light pulse reflected off a moving object. Terahertz waves sit between microwaves and infrared light.

A taut string sounds higher when you pull it tighter. Magnetization in an antiferromagnet behaves similarly: the stronger the external field, the faster it oscillates. But in chromium oxide crystals, something goes awry. In fields from 20 to 30 tesla, the resonance frequency grows more slowly than it should.

A shooter aims at a target, pulls the trigger, and hears two shots: one loud, one quiet. That's how the new setup works, except instead of bullets, there's an electron bunch, and instead of shots, there are two flashes of light. One flash is X-ray, the other is terahertz. They fly to the same point with perfect timing.

Light passing through a glass of murky water dims — some of it is absorbed. That's how many liquid-analysis instruments work: they measure how much light was lost and infer the composition from that. But if the liquid is heterogeneous, like soup with chunks, a single number isn't enough: you need to know where exactly more absorption happened.

A bell rings not from the strike but from a fleeting shudder of space. A gravitational wave, like ripples on a pond, passes through a massive magnet, and it deforms ever so slightly. That deformation can be turned into an electrical signal.

Throw a stone into water: right at the point of impact, the waves are chaotic — that's the near field. Farther out, they spread in smooth circles — the far field. This same principle governs antennas for terahertz communications — the future of super-fast internet.

A neat stack of atomic layers lies on a substrate. An invisible beam of terahertz light shines down on it, with a magnetic field applied from the side. After reflection, the beam's polarization rotates slightly.

An ordinary laser emits narrow lines, like a string that sounds only one note. For spectroscopy, this is inconvenient: if a substance absorbs light between the lines, you might miss it.

Gravitational wave detectors are microphones listening to the trembling of space. But their own noise drowns out weak signals. To hear more, physicists add special "squeezed" light to the instrument: it reduces quantum noise, like noise cancellation in headphones.

Dark matter is an invisible mass holding galaxies together. Its nature remains unknown, but one likely candidate is the axion — an ultra-light particle that barely interacts with matter. To catch it, physicists built a hybrid trap.

Radio waves that oscillate less than once per second pass through the earth and water with almost no loss. Such signals are used to communicate with submarines and to search for minerals. But a conventional antenna for them would need to be hundreds of meters long, and its sensitivity leaves much to be desired.

Light we can't see but feel as heat turns out to be the key to cellular life. A new type of microscope uses waves 2000–2500 nanometers long, three times longer than red light, and such waves barely scatter in tissue. Thanks to this, the device peers into a tumor spheroid like a flashlight through frosted glass, illuminating individual molecules.

Light hits a thin film, and an electric current instantly appears in it. This is how a pair of two materials works: molybdenum disulfide and cobalt. The first is a semiconductor, the second is a magnet. Between them, as it turns out, an invisible intermediary layer is born.

Even Einstein predicted gravitational waves — a trembling of the very fabric of spacetime. Today they are captured by gigantic installations like LIGO, created thanks to Rainer Weiss and Kip Thorne.

A blazing furnace in a workshop or the hot exhaust of a turbine is not just heat: it's light, invisible to the human eye. Regular solar panels catch visible light, but here you need a receiver for invisible thermal radiation.

Light in murky water behaves like a person in thick fog: every step is a collision, and the picture blurs. That's why a regular microscope can't see through skin or milk. Engineers found a workaround — look in the infrared range, where light collides less with particles.

An ordinary free-electron laser is like a musical instrument with a single string: it can play only one note until you change its design. To get a different wavelength, you have to retune magnets or accelerate electrons harder. That's expensive and bulky.

Light passing through a gas leaves narrow dark lines on the spectrum — the fingerprints of absorption. Acetonitrile molecules, like tiny antennas, respond only to strictly defined frequencies. But when there are many such lines and they are closely spaced, the signals overlap, like voices in a noisy room. As a result, clocks based on these molecules start to drift.

Light can be combed like hair. Instead of hair, we have frequencies; instead of a comb, a laser. The result is a comb made of thousands of even 'teeth'—frequencies. Such an optical comb helps study molecules and measure time with precision down to quadrillionths of a second. An ordinary comb has teeth spaced evenly apart.

Terahertz radiation sits between microwaves and infrared light. It passes through clothing, paper, and plastic but is blocked by water and metal. That's why these waves are used in security scanners and for quality control of materials.

The same explosion can sound different: it all depends on which way the wind is blowing. In 2024, researchers set off charges equivalent to ten tons of TNT twice and recorded the sound with a network of 31 microphones spread over a radius of 23 kilometers. The source was identical, but the acoustic pictures turned out to be quite different.

Terahertz radiation sits between microwaves and infrared light. It passes through clothing, paper, and plastic, but not through metal or water. That's why it's used in security scanners and medical imaging. To see the polarization of such radiation, you need a detector.

Pluck a guitar string, and it vibrates — the air around it carries the tremor to your ear. Spacetime vibrates differently: when a gravitational wave passes through, it stretches and squeezes slightly. Spotting such a tremor at frequencies from 10 kilohertz to 100 megahertz is the challenge that new detectors are being built for.

A warm cup or a human hand emits invisible light — mid-infrared radiation. Every substance absorbs this light in its own way, leaving a unique 'fingerprint'. From this fingerprint, you can tell what an object is made of without touching it. Previously, seeing this fingerprint required huge lasers that fired very short pulses. They were expensive and complex.

Terahertz waves sit between microwaves and infrared light. They pass through paper, plastic, and fabric, but not through metal or water. That makes them handy for inspecting packages without opening them or scanning luggage at the airport. But receivers for these waves have so far been made from pricey materials like gallium arsenide.

The electron is a tiny particle, but inside a crystal it behaves as if it had a different mass. Physicists call this the effective mass. To measure it, they make electrons run in circles in a magnetic field, like a speed skater on an ice rink who is kept from leaving the orbit.

There is a region of light that has long remained a blind spot: from 5 to 15 terahertz. It is not radio waves, nor infrared heat, but something in between, where molecules vibrate in particularly characteristic ways. Scientists from Germany have built a setup that finally peers into this 'new terahertz gap' and even beyond — past 25 terahertz. The secret lies in a crystal with the long name BNA.

A thin film of a bismuth-selenium compound sits on a substrate. A laser pulse lasting a millionth of a billionth of a second strikes it. Nearby, a magnet is switched on, with a field weaker than that of a fridge magnet.

In October 2022, the LHAASO observatory measured the spectrum (energy distribution) of gamma-ray burst GRB 221009A — the brightest on record. Its light traveled for two billion years and was so intense that it disturbed the upper layers of Earth's atmosphere.