HEP Experiment hep-ex

At Jefferson Lab, electrons are accelerated to 12 GeV and smash into protons to pry out their secrets. But existing detectors are like cameras with a narrow field of view: you either see a lot but dimly, or brightly but only a tiny patch. Electron scattering is the main tool, but statistics are insufficient for subtle effects.

At the Large Hadron Collider, millions of jets are born every second: streams of particles flying out from a single quark or gluon. Telling a jet from a top quark apart from a jet from an ordinary quark is a task on which the hunt for new physics depends.

In a dark laboratory where superconducting chips are cooled to thousandths of a kelvin, a qubit spins under the influence of a magnetic field. A regular qubit rotates in one direction. An antiqubit, its mirror twin, rotates in the opposite direction. Together they form a pair that senses the field twice as sharply as any ordinary pair.

A silicon sphere 166 nanometers in diameter floats in a beam of infrared laser light. The pressure is below 10⁻⁸ mbar, and the motional temperature is about 10 millikelvin. That is colder than the cosmic microwave background.

In 2016, the LHCb detector at the Large Hadron Collider recorded millions of proton-proton collisions. Among the debris of these collisions, neutral B mesons were born—particles that can spontaneously transform into their antiparticles and back.

Two muons are born in the decay of an eta meson and fly apart, linked by quantum entanglement. One experimenter, Alice, measures the spin of the negative muon, while another, Bob, records the direction of the positron from the decay of the positive muon. It would seem that the order of events should affect the correlations.

For 36 days, tropical cyclone Freddy raged over the Indian Ocean, the longest-lived cyclone on record. Meteorologists tracked it from satellites, aircraft, and ground stations. But one detail eluded all instruments: the precise air density deep within the vortex. And that density determines where the cyclone will turn tomorrow.

In 1976, Canadian physicist Bill Unruh asked a simple question: what does an observer see when accelerating through empty space? The answer turned out to be strange: emptiness ceases to be empty. An accelerating observer bathes in thermal radiation with a temperature proportional to the acceleration.

In 1936, two physicists, Werner Heisenberg and Hans Euler, poring over the equations of quantum electrodynamics, found something strange. In a sufficiently strong magnetic field, vacuum should cease to be empty.

The muon is a tiny spinning top, twirling in the turbulent sea of the vacuum. Its magnetic axis points slightly away from what the Standard Model predicts. The deviation is just a couple of parts per million, but for physicists, it's a full-blown mystery. The vacuum is not a dead calm.

At the DESY lab, the ALPS II experiment was launched to hunt for axions — hypothetical ghost particles that might make up dark matter. This invisible mass acts like a skeleton, preventing galaxies from flying apart due to their spin.

Dark matter makes up 85% of the matter in the Universe, yet remains invisible. It only reveals itself through gravity. We can catch it by its cosmic 'hum' — a faint vibration that permeates space. A single detector is powerless here: the signal is too quiet. Physicists turn many sensors into a quantum ensemble.

Our Sun emits streams of neutrinos — particles that barely interact with matter. Passing through the dense solar material, they change their type — scientists call this 'flavor.' It's like a voice that changes as it moves through a crowd: the thicker the crowd, the more it gets distorted.

Neutron stars are the compressed remnants of massive stars: their matter is squeezed so tightly that a thimble-sized amount would weigh a colossal amount. If dark matter, the mysterious invisible substance thought to hold galaxies together with its gravity, accumulates inside such an object, under certain conditions this accumulation becomes fatal.

Inside a giant spectrometer in Karlsruhe, shaped like a huge metal barrel, scientists are catching particles that are nearly impossible to catch. Neutrinos are the ghosts of the microcosm: every second, trillions of these particles fly through your body, and you don't even notice. But they do have mass, and scientists want to measure it.

In a dark room, there is a tank of liquid argon. Sometimes an invisible particle flies through it, strikes an atomic nucleus, and a faint light flashes in the liquid. From this flash, physicists try to figure out what kind of guest has arrived.

Dark matter is invisible, but according to calculations, it holds galaxies together. Catching its particles is like hearing a whisper in a noisy room. You need a material that responds loudly and noticeably to the slightest nudge. Molecular magnets could be such a material — substances where each molecule acts as an independent tiny magnet.

Dark matter is an invisible substance, five times more abundant in the universe than ordinary matter. Its particles barely touch atoms, but occasionally they can nudge an electron, like a string brushed by the wind.

Neutrinos are the most elusive of all known particles. Every second, trillions of neutrinos from the Sun fly through your body, but you never notice: they barely interact with matter. To catch even one, physicists build giant detectors — pools of water or liquid argon deep underground.

In a dark room, you might notice a faint blue glow around some radiation sources. This is Cherenkov light: it appears when a charged particle travels through a medium faster than light can propagate in it. The result is a light shock wave, similar to the sonic boom from a supersonic jet, but made of photons.

Two black holes circle each other, and their dance isn't always a smooth waltz. If the holes spin on their own axes, their orbit can start to tumble, like a top that's been pushed and wobbles on its side while still spinning.

Dark matter is five times more massive than ordinary matter, yet it emits no light. Its nature remains unknown. One candidate is the ultra-light axion particle. Axions could pierce right through the planet, barely noticing atoms.

Two spinning tops are set off simultaneously in opposite directions. If one spins left, the other always spins right — no matter how far apart they fly. That's roughly how quantum entanglement works, except instead of tops, we have top quarks, the heaviest known particles.

Inside protons accelerated to nearly the speed of light, a particle heavier than a gold atom is sometimes born — the top quark. It lives for tiny fractions of a second and decays, leaving a trace in the ATLAS detector. Physicists collected such traces for four years to understand how often the top quark and its mirror twin, the antiquark, appear.

Water in a kettle heats to 100 degrees, and stops being water, turning into steam. Something similar happens to atomic nuclei when they are smashed together at enormous speeds in the Large Hadron Collider.

Dark matter is an invisible substance that holds galaxies together but emits no light. Catching its particles is like trying to hear a whisper in a noisy hall. Ordinary detectors only pick up loud impacts, while weak signals get drowned out by background noise.

A pebble drops into a pond, and ripples spread across the water. But sometimes the pebble doesn't sink right away: it skims beneath the surface, travels a few meters, and only then surfaces, creating ripples in an unexpected spot.

Deep inside an underground laboratory, a room-sized detector waits for an event that might happen once in a hundred million billion years. That event is neutrinoless double beta decay — a process that would break one of physics' fundamental laws. To catch it, you need perfect silence: not a single stray radioactive atom in the detector's materials.

Inside a large particle accelerator, an invisible shower of gamma rays reigns, like leaving a glass thread under an X-ray machine switched on for years. Ordinary electronics there quickly fail, yet data from the detector still needs to get out. The solution is optical fiber: a thin glass core that carries light.

The cosmos is filled with invisible dark matter, which betrays itself only through gravity. Its existence was suspected by Fritz Zwicky and confirmed by Vera Rubin.

The LCLS-II X-ray laser in California fires short, powerful flashes, like a strobe light at a disco. Between flashes, there are dark pauses lasting 26.9 nanoseconds (billionths of a second).

In the BESIII detector, particles put on a show: they collide, are born, and decay, leaving flashes of light. But sometimes an actor can leave the stage unnoticed — through a hidden door that cameras don't see. Physicists were looking for exactly such 'quiet' decays, when a particle turns into something invisible to the instruments.

Every atom has its own 'voice'—the frequency of light it emits. For isotopes, atoms with different numbers of neutrons, the voices differ slightly. It's like a choir: if you know the score precisely, the slightest false note reveals external interference. The King plot is a way to compare how harmoniously two notes from different isotopes sing together.

When a top quark is born in a particle detector, it immediately decays into a shower of other particles. Catching a hint of new physics in that shower is like hearing a whisper at a rock concert. You need not just a good microphone, but the ability to subtract the roar of the amplifiers and the hum of the crowd.

Inside a refrigerator that cools matter to near absolute zero beats a mechanical heart — the pulse tube. It pumps gas and extracts heat, but along with the cold it brings tremors. Each beat of this heart shakes the instruments sitting next to the sample and ruins delicate measurements.

An ordinary piece of germanium the size of your palm can spot a single dark matter particle flying through it. But for that, the crystal must be nearly perfect: free of electrical noise, with a uniform internal field, and contacts that don't spark at high voltage. In the new work, they assembled the KL01 detector.

A muon is like an electron, but 207 times heavier. When it slams into matter, it slows down like a bullet in a sandbank, and at every bend in its path it emits X-rays. Those X-rays tell you which atoms the muon encountered: that's the idea behind a technique called MIXE. It lets you peer inside an object without dismantling it, like an X-ray for materials.

In the Large Hadron Collider's detector, each proton collision leaves thousands of points — tracks of flying particles. A neural network learned to spot patterns in this scatter and predict what happened at the moment of impact.

Diamond is not just a gemstone. This crystal can conduct electricity when free charge carriers, electrons and holes, appear in it. But how fast do they move? In scientific papers, numbers vary by tens of times. One lab reports a mobility of 1000 cm²/(V·s), another 4000.

At a particle accelerator in Beijing, electrons collide with positrons, and for a fleeting moment, a particle called eta-c is born. It lives for a tiny fraction of a second and then decays into other particles. One of the rarest paths is to split into two photons, particles of light. Until now, no one could say exactly how often this happens.