silicon detector

A particle enters a silicon wafer like a courier arriving in an unfamiliar city: it must not only deliver its signal but also leave an accurate record of when it arrived. The 3D sensor on the Timepix4 chip makes that record to within 245 picoseconds, and it pinpoints the meeting spot to just 7 micrometers.

The antiproton beam hits the plate, and each impact bursts into a shower of charged particles. In the GBAR experiment at CERN, this picture is captured not by a sophisticated detector but by an ordinary industrial camera without a lens, pressed against the vacuum window from the outside.

A globe sits on a table, and a ruler lies beside it: one is curved, the other straight. X-ray telescopes have lived with this mismatch for years. Their mirrors gather light onto a curved surface, like the globe, while the detectors that catch that light have been flat, like the ruler.

A single photon is like a perfectly smooth brick from which quantum technologies can be built. But to build a house, you need thousands of identical bricks. Rubidium atoms are natural emitters: each atom emits photons of exactly one wavelength, like a tuning fork that always produces a single note.

In an ordinary room, light vanishes the moment you switch off the lamp. In a tiny silicon nitride cavity, a photon can bounce between the walls 80,000 times before it gets lost. It's like a ball thrown into a room that rebounds off the walls with almost no loss of speed.

A passing particle leaves a flash of light in a long transparent bar — a scintillator. Inside the bar, like threads in a rope, thin fibers are stretched to collect this light and channel it to a sensor. Particle detectors have worked this way for decades.

To probe deeper into the workings of the universe, physicists accelerate electrons and smash them together. An ordinary electron is like a spinning top that wobbles randomly. For delicate experiments, you need particles whose spins all point in the same direction: this is called polarization.

Usually, light does not turn an insulator into a conductor: that requires powerful laser pulses that break the material's structure. But in twisted bilayer graphene at the magic angle, things are different.

Dark matter detectors are essentially incredibly sensitive microphones, capable of hearing a whisper amid the roar of a rock concert. Their job is to catch the rare nudges from hypothetical dark matter particles, which are thought to occasionally collide with atomic nuclei of ordinary matter.

A flashlight beam aimed through frosted glass turns into a blurry spot with every extra millimeter of thickness. Scintillators, materials that convert X-rays into visible light, behave much the same way. They underpin medical imaging, baggage screening, and detectors at particle accelerators.

A detector filled with superfluid helium-4 is like a perfectly still lake. The liquid doesn't slosh or bubble: it's frozen in a single quantum state. An invisible guest, a dark matter particle, flies through it. It doesn't shine or leave a track. But sometimes it nudges a helium nucleus.

Light leaves a trace even when there is almost none of it. A single photon, a tiny bundle of energy, strikes a silicon wafer and knocks out a handful of electrons. The trouble is that the handful is too small to notice. You need an amplifier. Usually, the signal is amplified by applying a voltage to metal contacts on the detector's surface.

Silicon carbide is the material used to armor electronics. It withstands heat, impacts, and radiation like the ceramic tiles on a spacecraft's heat shield. But even this armor has a weak spot: ordinary metal contacts quickly degrade under X-rays.

When two particles fly at almost the same speed in the same direction, their signals in the detector merge, like two voices in unison. Telling a duet from a soloist is an art in itself.

Light in a particle detector behaves like a voice in the mountains. One shout, and the echo repeats several times, growing fainter with each reflection. So it is in a silicon detector: a real flash from a particle gives rise to false ones that confuse measurements.

In giant accelerators, particles zip through detectors in billionths of a second, and telling one from another requires a stopwatch of incredible precision. The new µRWELL-PICOSEC detector acts as such a stopwatch: it captures the moment a particle passes with a precision of 48 picoseconds: that's 48 trillionths of a second.

A security guard needs to check five rooms but can't go inside. He knocks on the door and listens: silence means someone is inside, while an echo means the room is empty.

Inside an ultra-thin polymer thread are microscopic crystals — scintillators. When an invisible radioactive particle hits, they flash for a moment, like fireflies. A sensitive sensor catches each flash, turning the thread into a flexible detector.

Plain water in a glass is clear and calm. But if you add tiny carbon dots made from sugar and citric acid in an ordinary microwave, the water starts to glow when a charged particle flies through it.

Light in an optical fiber is a stream of photons, and quantum communication requires single photons that can be sent one at a time. But making them emerge quickly while remaining indistinguishable from one another is a tough challenge.

Underground, in a former gold mine, sits a tank of liquid xenon. If a dark matter particle flies through it, the xenon flashes. But it also flashes from ordinary particles, like neutrinos or leftover radioactivity. The task is to tell which flash comes from dark matter and which from noise.

A single electron in a magnetic field is like a tiny top that spins and weakly "squeaks" at its own frequency. Hearing that squeak directly is nearly impossible: it gets lost in the noise. Scientists have devised a resonator: a superconducting microwave strip that works like a tuning fork tuned to the same note.

The camera that hunts for tumors works like a highly sensitive camera: it catches the faint glow from a substance that accumulates in diseased cells. In conventional machines, the light is born in a crystal — a solid piece that resembles glass. But a crystal doesn't always convey exactly where the light flashed, so the image comes out slightly blurry.

In a dark tank holding thirty tons of water, the liquid glows when a ghostly particle streaks through. Neutrinos barely interact with matter, but occasionally they bump into atoms, and a flash is born. To catch it, a special substance, a liquid scintillator, is added to the water to amplify the light.

In a particle accelerator, nuclei shatter into fragments like a porcelain cup dropped on the floor. Each fragment flies through silicon wafers, which register the impact and its strength. But to distinguish a real signal from random noise, you need a threshold: below it, readings are considered interference.

The future neutrino detector will contain millions of tiny plastic cubes: each the size of a die. They flash when a ghostly particle passes through, and that flash must be captured and measured. But if a cube is warped, has a burr, or a hole in the wrong place, the signal gets distorted, and the detector starts lying. Checking each cube by hand is like sifting through sand on a beach.

Tuning a radio to your favorite station is a search for the right frequency amid the noise. The new device does the same, but for waves about three millimeters long. Such waves come from distant galaxies and possibly from dark matter particles. The device is a pattern of superconducting niobium traces on a silicon wafer.

A tiny glass sphere floats in a laser beam like a speck of dust in sunlight. Inside it is radioactive lead, which decays from time to time. Each decay ejects charged particles, and the sphere loses or gains a tiny electric charge.

A power transistor made of silicon carbide operates under voltages thousands of times higher than what comes out of a wall outlet. If the field inside it becomes uneven, the device burns out. Previously, this field was invisible: it is too strong for ordinary sensors, and the device must remain under voltage.

Radio waves surround us, but our eyes can't see them. This new sensor, the size of a fingernail, turns them into a colored patch on a tiny screen. Inside the chip is a layer of liquid crystals — the same kind used in phone displays. Among them are embedded thin ferromagnetic nanowires. When a radio wave arrives, the nanowires heat up quickly.

A quantum computer is like an orchestra, where each qubit is a musician playing their part. But every now and then, a cosmic ray bursts into the hall, and the violinist flinches, losing the rhythm. These particles from deep space pierce the chip, knock out extra electrons, and spoil the delicate quantum music.

The receiver doesn't catch radio waves but submillimeter light — the radiation emitted by cold clouds of gas and dust in distant galaxies. Inside, there's an array of tiny resonators, each tuned to its own frequency, like the strings of a grand piano tuned to notes.

In an ordinary light bulb, light is born when an electron and a hole meet. In the new material, they are deliberately pushed apart, as if a turnstile were placed between them at a subway station. This turnstile is a built-in electric field that arises because sulfur and selenium atoms in the crystal are arranged asymmetrically: sulfur on top, selenium on the bottom.

When treating epilepsy, doctors adjust the drug dose almost blindly. Too little, and seizures continue; too much, and side effects appear. Usually, a patient's blood is sent to a lab, and the result comes back a day or two later. Now, the same test can be done on a tiny silicon chip. The sensor works like a highly sensitive nose.

The tip of a scanning tunneling microscope approaches a crystal surface so closely that an electric current jumps between them. Electrons from the needle are injected into a layered semiconductor and land in an atomic vacancy — a spot where one atom is missing from the lattice. This void acts as a tiny trap for charge.

The night sky is not all that dark. Even far from cities, it glows faintly — which hampers astronomers trying to catch weak flashes from distant cosmic rays.

A particle zips through silicon in billionths of a second, and the sensor manages to click, recording the exact time. This isn't science fiction; it's the result of testing the MiniCACTUS-v2 prototype at CERN in July 2025. The best result: 48.88 picoseconds — in that time, light travels just 1.5 centimeters.

When a particle zips through a transparent material faster than light can travel through it, it leaves behind a faint blue flash, just as a jet breaking the sound barrier creates a shock wave. This Cherenkov radiation fires instantly, with no delay, making it perfect for ultra-precise timing in the world of elementary particles.

The universe is held together by an invisible scaffolding of dark matter. Part of it could be dark photons, ghostly copies of light that pass right through matter. The Dandelion experiment turned a spherical mirror into a super-sensitive ear: it gathers dark photons and translates them into the language of radio waves.

A camera that captures not light but a stream of electrons reflected off a crystal is a hybrid pixel detector. It can count every electron that hits it, generating almost no noise of its own. In normal mode, when the electron beam flows continuously, the detector works perfectly.