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underground laboratory

A facility built deep underground to shield sensitive detectors from cosmic rays and background radiation.
8 related articles

Description

An underground laboratory is a research facility built deep beneath the Earth's surface, often in mines or caverns, to shield sensitive experiments from cosmic rays and other background radiation. Cosmic rays — high-energy particles from space — constantly bombard the surface, creating a noisy background that can swamp the faint signals physicists seek to detect. By placing detectors hundreds or even thousands of meters underground, the surrounding rock absorbs most of this radiation, providing a quiet environment for studying extremely rare events.

History

The concept emerged in the 1960s, when physicists began placing detectors deep underground to study neutrinos and search for proton decay. Early examples include the Homestake experiment in South Dakota, which began operating in 1967.

How it works

The overlying rock acts as a natural shield. When cosmic rays hit the atmosphere, they produce showers of secondary particles; the deeper the lab, the fewer of these particles penetrate. The rock also blocks gamma rays and neutrons from natural radioactivity in the environment. Labs are typically built in stable geological formations, with additional layers of shielding — such as lead or copper — inside the cavern to further reduce background noise.

In practice

Underground laboratories host experiments in neutrino physics, dark matter detection, and rare nuclear decays, such as the search for neutrinoless double beta decay.

Fun fact

The deepest underground laboratory, the China Jinping Underground Laboratory, sits under 2,400 meters of rock, reducing cosmic ray flux by a factor of about 100 million.

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Related articles · 8

A Trap for the Invisible
Deep inside a mountain, where cosmic-ray muons are muffled by a thick layer of rock, stands a detector that catches not light but its absence. Positronium is a tiny atom in which an electron and its antiparticle, the positron, circle each other like a pair of dancers. Usually they come together and vanish in a flash of two or three gamma quanta.
HEP Experiment2026-08-091 minarXiv:2608.08592express
A Detector That Can Hear the Universe's Whisper
The universe is constantly sending us signals, but many are too faint to notice. Relic neutrinos, particles left over from the Big Bang, pass through Earth by the billions every second, yet catching even one is a feat on the edge of possibility. We need a detector that can sense energy a thousand times smaller than what it takes to move a speck of dust.
Cosmology2026-05-031 minarXiv:2605.01994express
Cosmic voids are not quite empty
The Universe is structured like a sponge: there are dense regions packed with galaxies and gas, and giant pores — cosmic voids. These voids occupy most of space, but their contents have remained a mystery because matter there barely reveals itself. Now astronomers have 'felt' the voids using fast radio bursts — super-powerful pulses from distant galaxies.
HEP Experiment2026-02-241 minarXiv:2602.21177express
Radon Hides Dark Matter
A dark matter detector is like a room where you're trying to hear a whisper while static electricity crackles nearby. This crackle is produced by radon atoms — a radioactive gas that seeps out from materials and air.
Quantum Physics2026-02-061 minarXiv:2602.06352express
A Laser from the Moon's Eternal Shadow
At the bottom of lunar craters, where sunlight never reaches, an eternal cold reigns — about minus 240 degrees Celsius. In these icy pockets, known as permanently shadowed regions, plans are underway to install a mirror resonator made of monolithic silicon.
HEP Phenomenology2026-01-221 minarXiv:2601.16259express
Dark Matter: Why It Hides from Us Behind the Atmosphere
Since Vera Rubin first convincingly showed that galaxies are surrounded by invisible matter, the quest to understand the nature of dark matter has remained one of physics' greatest challenges.
Quiet Silicon for Ghost Hunting
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.
Exoplanets2025-12-102 minarXiv:2512.09660express
A Nearby Supernova: How Rocky Planets Are Born
Just as yeast turns flour into fluffy dough, radioactive 'seasoning' from a supernova — the explosion of a massive star at the end of its life helps mold a rocky planet. The key ingredient here is aluminum-26, a radioactive isotope that releases heat as it decays.