decay time

A drying puddle of mud becomes covered with cracks, like an old painting with craquelure. At first the cracks meet at nearly right angles, forming a rough grid. But if the mud is wetted again and allowed to dry, the pattern changes: cracks begin to meet in threes, at an angle of 120 degrees, like a honeycomb. Why this happens remained a mystery for a long time.

A perovskite solar cell is like a young athlete: it performs brilliantly at first, but tires with age. Over eight hours, its performance drops noticeably, with no visible cause like cracks or dust. Scientists took one cell and recorded its performance at 0, 90, 280, and 480 minutes of its life.

A hunter sets snares in the woods. They know the animal's habits but not whether it will ever show up. In much the same way, physicists set up detectors in hopes of catching particles of dark matter — the invisible substance thought to make up most of the Universe's mass. A new study offers hunters an unusual tool: not a trap, but a measuring tape.

The Sun is constantly struck by blows — magnetic reconnection in the plasma releases energy, making the corona flare up. After each such blow, magnetohydrodynamic waves linger in the plasma loops, like the fading ring of a bell.

A coin landing on its edge is about as rare as a heavy B meson decaying into a light pion and an electron-positron pair. Over a decade of collider operation, only a handful of such events have accumulated, but physicists have finally managed to spot them. The decay probability is about 2.4×10⁻⁸.

In 2017, the IceCube detector caught a neutrino from the distant galaxy TXS 0506+056. It was like hearing a phone ring from across the ocean: the signal came from where the most energetic particles in the Universe are born. At the same time as the neutrino, astronomers spotted a gamma-ray flare, and two to three years later, radio waves. Why was the radio late?

Dark matter is an invisible substance that keeps galaxies from flying apart. If its particles occasionally decay near the Sun, they shoot out streams of fast particles, like invisible hammers striking light. Each impact turns a particle of sunlight into a gamma ray — a super-powerful flash that telescopes can spot.

For 17 straight years, the Fermi space telescope recorded light from the distant galaxy 4C 76.03. Most of the time, it behaved quietly, like a night city with only a few lit windows. But in the observation archive, two brief moments stood out when the galaxy flared in gamma rays — the most energetic light in the universe.

Twenty-eight seconds: that's how long it took for an automated camera to lock onto a flash in a constellation whose light had traveled for more than nine billion years.

A solar flare is like a short circuit in a giant neon sign. Inside the Sun, magnetic fields twist into loops, like rubber bands, and when they reconnect, energy bursts into space. Part of it goes into hard X-rays, produced by particles accelerated to nearly the speed of light.

A solar flare is like a tightly coiled spring suddenly uncoiling. In the Sun's corona, energy accumulates in the twisted magnetic field, and then it is abruptly released, accelerating particles and heating plasma.