HALO
IP-2 · GENERAL PURPOSEAn onion of instruments, 24 m across. If something new is made at Meridian, HALO is built to notice — this is where the axion-9 search lives.
MERIDIAN COLLIDER · RUN 88 · STABLE BEAMS
Twenty-seven kilometres of superconducting ring beneath the Val Brenga. Two beams, forty million crossings a second — and somewhere in the debris, we think, a particle nobody has ever seen.
CLICK / TAP ANYWHERE — TRIGGER AN EVENT
EVENT READOUT — IP-2 (HALO)DAQ OK
EVT 0408 · E=13.1 TeV · 57 tracks · axion-9 candidate: no
EVT 0407 · E=12.8 TeV · 44 tracks · axion-9 candidate: no
Under an alpine valley, two beams of protons travel a ring the length of a marathon at 99.999996% of the speed of light — one clockwise, one counter-clockwise. Where they cross, protons meet with the energy of two head-on freight trains packed into a space a trillion times smaller than a raindrop. Everything below is kept colder than deep space, so the magnets that steer the beams lose no energy at all.
A collision lasts about a hundredth of a billionth of a billionth of a second. The detectors are how we replay it. Each is a camera built for a different question — hover or tab through the layers to see what each shell does.
An onion of instruments, 24 m across. If something new is made at Meridian, HALO is built to notice — this is where the axion-9 search lives.
Looks down the beam instead of around it. VETRA watches particles that barely deflect — the shy ones — and times them to a trillionth of a second.
A 3,000-tonne stack of steel and scintillator that measures what isn't there. If energy leaves a collision unseen, CASCADE notices the hole it left.
The quiet one. No beam at all — a supercooled cavity listening for axion-9 drifting in from the galaxy, faint as a radio station one photon strong.
Every programme at Meridian is public from day one. Data is embargoed for exactly ninety days — after that, anyone on Earth can download it.
Four-fifths of the matter in the universe is missing. We can weigh it — galaxies spin as if held by something enormous and invisible — but nobody has ever caught a piece of it.
Axion-9 is our best guess: a particle so light that a billion of them would weigh less than a single electron, drifting through the valley, through the mountain, through you, right now. It almost never touches ordinary matter. Almost is the word this laboratory is built on.
In March 2026, the AXIA team found 14 collisions that look like axion-9 being born: two photons and a hole in the energy books, exactly where theory said to look. Fourteen events is a whisper, not a discovery — chance could fake it roughly once in two hundred tries. We need about forty more. At current beam intensity, the answer arrives in eleven months. You can watch the counter move on this page.
Four times a year, we hand a badge, a desk in the HALO control room, and full data access to someone who doesn't work here — an early-career physicist, a teacher, once a glaciologist who wanted to apply her avalanche statistics to particle showers. (It worked. She's on two papers.)
Residents take shifts, break things, fix them, and leave with their name in the logbook. No publication quota, no deliverables. The only requirement is a question you can't stop thinking about.
“I expected a cathedral. It's more like a ship — everything hums, everyone has a station, and the night shift makes the best coffee in the canton.”
On open days we take you down: the lift, the tunnel that curves away farther than you can see, the control room where the event counter never stops. Children under 12 get their own dosimeter badge to keep. (It reads zero. That's the point — and the physicists will happily explain why.)
NEXT OPEN DAYS
SAT 05 SEP 2026 · 09:00–17:00 — RING & HALO CAVERN
SAT 03 OCT 2026 · 09:00–17:00 — RING & CASCADE HALL
AUTUMN OPEN WEEKEND · 24–25 OCT 2026 — ALL FOUR DETECTORS
Autumn allocation opens 01 AUG 2026, 06:00 CET. 240 places per day, free of charge. Bring warm layers — the tunnel holds at 17 °C all year.