substance

manganese

A chemical element used in molecular magnets for dark matter detection.
21 related articles

Description

Manganese is a chemical element (symbol Mn, atomic number 25) that plays a crucial role in various advanced technologies, including the construction of molecular magnets used in dark matter detection experiments. These molecular magnets are nanoscale clusters of atoms that exhibit magnetic properties at low temperatures, and they are being explored as sensitive detectors for weakly interacting massive particles (WIMPs), a leading dark matter candidate. Manganese's specific electronic configuration and magnetic properties make it a key component in these systems, where it helps create the strong internal magnetic fields needed to detect the tiny energy signatures of dark matter interactions.

History

Manganese was isolated as an element in 1774 by the Swedish chemist Johan Gottlieb Gahn. Its use in molecular magnets for dark matter detection is a recent development, emerging in the 2010s as part of the search for alternative detector technologies.

How it works

In a molecular magnet for dark matter detection, manganese ions are arranged within a larger molecular structure, creating a system with a large total spin and magnetic anisotropy. When a dark matter particle collides with the molecule, it can cause a spin flip or a change in the magnetic state, releasing a detectable amount of energy. The detector is cooled to extremely low temperatures to minimize thermal noise, and the energy released is measured via changes in magnetization or heat capacity. Manganese's role is to provide the magnetic moments that make the system sensitive to these rare interactions.

In practice

Beyond dark matter detection, manganese is widely used in steel production (as an alloying agent), in batteries (e.g., lithium-manganese oxide cathodes), and in pigments and fertilizers.

Fun fact

Manganese is essential for human health, playing a role in bone formation and metabolism, but excessive exposure can cause a neurological disorder called manganism, which resembles Parkinson's disease.

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Related articles · 21

A Crystal Trap for Light Dark Matter
No one has ever seen dark matter, but it should pass through detectors like wind through leaves. Sometimes, very rarely, a dark matter particle bumps into an atomic nucleus, and then the detector must catch that jolt. The trouble is that light dark matter particles can hardly move heavy nuclei: it's like trying to knock down a bowling pin by throwing a feather at it.
Cosmology2026-07-262 minarXiv:2607.23527
Wind from Cygnus: First Directional Limits from MIMAC
264 kilometres per second — that's how fast the Solar System hurtles through the cloud of dark matter. Its existence was given away by galaxies: they spun too fast to be held by visible mass, and Vera Rubin was first to suspect a hidden scaffolding.
Dark Weather over Gran Sasso: Daily Rhythm of Sub-GeV Dark Matter
At nine in the morning, the DarkSide-50 detector, 1400 meters beneath Gran Sasso, records a weak ionization pulse. By eleven at night, the frequency of such events drops noticeably. This is not an electronics glitch or a seasonal background variation.
Quantum Physics2026-06-171 minarXiv:2606.18871express
Tiny Diamond Compass Peers Inside Batteries
Ordinary magnetic sensors lose sensitivity as they shrink. But scientists turned a tiny diamond into a light-based compass. Unlike jewelry diamonds, what matters here isn't purity but artificially created defects — these are what turn the crystal into a compass.
Lead Archives: Ancient Minerals vs. Higgsino
The story began almost a century ago, when Edwin Hubble showed that galaxies are receding, and Fritz Zwicky and Vera Rubin later realized: to explain their motions, invisible mass is needed — dark matter.
HEP Phenomenology2026-05-292 minarXiv:2606.00237express
How to Catch Dark Matter with a Wave
Drop two pebbles into a pond at the same time — the ripples will spread evenly and in sync. The same happens in a quantum interferometer: a particle is split into two waves that travel along different paths and then meet. Ideally, their crests align.
HEP Phenomenology2026-05-272 minarXiv:2605.28275express
A Neutrino Whisper from the Dark Sector
Deep underground in Japan, a huge tank of ultrapure water waits for rare visitors — neutrinos arriving from distant stellar explosions. Such guests are few and far between: over years of observation, Super-Kamiokande registers only a handful of events.
Materials2026-05-242 minarXiv:2605.25241express
Magnetic Patterns at the Atomic Level
Two magnets on a table either attract or repel — depending on how their poles are oriented. Inside each piece hide tiny regions where all the magnetic arrows point in the same direction. These regions are called domains, and their arrangement determines how the material behaves in an electrical circuit. In altermagnets, a new class of materials, domains are trickier.
High Energy2026-05-191 minarXiv:2605.19653express
Invisible Middleweight Black Holes Discovered
Black holes come in lightweights, born from dying stars, and supermassive ones at galactic cores. The missing intermediate link had been hiding. Fast radio bursts, cosmic signals lasting milliseconds but carrying the energy of days of sunlight, helped crack the case. Think of these bursts as cries from the depths of the universe.
Galaxies2026-04-292 minarXiv:2604.26439express
Record-Breaking Cloud: How TMC-1 Doubled Our Chemical Inventory
A giant cloud of gas and dust, so cold that its warmth barely flickers, just a few degrees above absolute zero. This is TMC-1 in the constellation Taurus, one of the darkest and densest cradles of molecules in our Galaxy. In recent years, it has become a true treasure trove for astrochemists: the number of substances found there has more than doubled.
Galaxies2026-04-272 minarXiv:2604.24510express
The Scent of the Universe: Benzene Rings in Hot Clouds
In dark, cold clouds of interstellar gas, astronomers have for several years been spotting aromatic molecules — compounds built around a benzene ring (a hexagon of carbon atoms), like the benzene we know. One such substance, benzonitrile (benzene with a cyano group attached), had only been found in very calm and cold places, like the Taurus cloud.
Stellar2026-03-122 minarXiv:2603.11945express
The Hidden Magnets of White Dwarfs
A white dwarf is what remains of a star like the Sun after it sheds its outer layers. What's left is a hot core the size of Earth but with a mass close to that of the Sun. A teaspoon of this material would weigh as much as a truck. Some of these stars have extremely strong magnetic fields — a billion times stronger than Earth's.
Galaxies2026-03-012 minarXiv:2603.01041express
A Chemical Map of a Starry Swarm
At the heart of Omega Centauri, the most massive globular cluster in our Galaxy, thousands of stars are packed so tightly that their light merges into a single glowing blob when seen from Earth. Separating this swarm into individual stars and determining the composition of each is a task akin to sorting through an overfilled anthill.
HEP Phenomenology2026-02-192 minarXiv:2602.17620express
A 17 MeV Ghost Particle
In nuclear transitions of beryllium-8, helium-4, and carbon-12, physicists from the ATOMKI collaboration have been seeing extra events since 2020—as if, when an excited nucleus decays, something else is sometimes born besides the usual photons. The energy of this "something" is always the same: about 17 million electron-volts.
HEP Experiment2026-02-102 minarXiv:2602.09421express
Heavy Dark Matter: Traces in Liquid Argon
A bullet that doesn't just pierce one target but leaves marks in several layers of armor. That's roughly how superheavy dark matter behaves, and it's what the DarkSide-50 detector was built to catch for the first time. The usual suspects for dark matter (weakly interacting massive particles, or WIMPs) pass through matter almost unnoticed, occasionally bumping into a nucleus.
Lead from an Ancient Shipwreck Hunts Dark Matter
Ancient lead that lay on the seafloor for two thousand years has become the heart of a detector searching for the most elusive substance in the universe. From it, researchers grew a transparent lead tungstate crystal weighing 13 grams and cooled it to near absolute zero.
Materials2026-01-181 minarXiv:2601.12623express
Crystal Timekeepers: How Molecules Sense Magnetic Fields
Magnetic fields are all around us, from the compass in your phone to the MRI machine at the hospital. To measure them with high precision, you need special materials that respond to the slightest changes in the field. One such material is molecular crystals, where electron spins, think of them as tiny tops, can hold their state for a long time.
Cosmology2026-01-041 minarXiv:2601.01340express
Dark matter isn’t so cold after all
The enigma of dark matter was already studied by Fritz Zwicky and Vera Rubin. For decades, it was depicted as a cold, listless skeleton that only draws galaxies together.
HEP Phenomenology2026-01-031 minarXiv:2601.01043express
Molecular Magnets Catch Dark Matter
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.
HEP Phenomenology2025-11-252 minarXiv:2511.20461express
Porous Crystals as Dark Matter Detectors: Catching the Phonon Whisper
In the 1930s, Fritz Zwicky, observing the Coma cluster, noticed anomalously high galaxy velocities: their motion pointed to a huge hidden mass gravitationally binding the system.
Materials2024-10-213 minarXiv:2410.15776
Cold from Iron: How a Cheap Alloy Replaces Rare-Earth Magnets
The temperature in a room drops by a few degrees while the refrigerator runs without a single moving compressor. Inside, there is no Freon, but a piece of metal that is alternately magnetized and demagnetized.