Everything around us — not just light, but also matter particles, such as electrons — behaves like waves! Every moving particle has its own wavelength, calculated using the de Broglie formula. For large objects, this wavelength is vanishingly small, so we don't see a ball bending around corners. But for tiny particles, it is large enough to exhibit wave properties.
History
Louis de Broglie in 1924 suggested the universality of wave-particle duality, extrapolating the results of Planck and Einstein for light to all particles. In 1927, Clinton Davisson and Lester Germer experimentally discovered diffraction of slow electrons on nickel, and George Thomson in thin metal films. These experiments confirmed the hypothesis, and Erwin Schrödinger soon developed the mathematical apparatus to describe de Broglie waves.
How it works
The de Broglie formula is used to calculate diffraction gratings in electron and neutron optics, estimate quantum effects (tunneling, interference) during microparticle motion, and in scattering theories. In the macroscopic limit (m large), λ becomes negligibly small, consistent with classical mechanics. For ultra-relativistic particles, a relativistic expression for momentum is required.
Fun fact
If you throw a baseball, its de Broglie wavelength would be billions of times smaller than an atomic nucleus — no diffraction would be noticeable. But for a slowly moving electron, it can be the size of a molecule!
A thrown stone sends ripples across water. A gravitational wave is the same kind of ripple, but in spacetime. It is produced, for example, by the merger of two black holes. In classical physics, this ripple is eternal: once created, it travels through the Universe without fading.
Eight bright spots on the radio sky. They are all the same quasar HS 0810+2554, whose light passed through a gravitational lens — a massive foreground galaxy.
A shock wave is like a steep wall of water rolling down a calm river. In physics, such waves arise when matter is compressed faster than the signal about that compression can spread sideways. In ordinary water or air, things are more or less clear.
In water cooled to –40°C, a paradoxical pause sets in: perfect hexagonal ice is in no hurry to form. Instead, a disordered structure with interspersed cubic layers emerges — a real cradle for future symmetry, brimming with disorder yet already charged with hidden architecture.
Strike a tuning fork. The frequency is 440 Hz. That's the note A — the standard of sound.
In the world of numbers, there's a standard too. It's tuned not to sound, but to prime numbers. Though their distribution seems random, it obeys strict laws. All primes resonate together. There's just one value: λ∞ ≈ 0,674036.
A stone falls into water, and ripples spread in all directions. Throw a handful of stones at once, and the ripples overlap: you can no longer tell which ripple came from which stone. A neutron beam hitting a detector looks much the same: a bright spot blurred by many causes.
Toss a handful of phosphorus into silicon, and at a certain impurity concentration the material suddenly starts conducting electricity. This is a metal-insulator phase transition, and it happens abruptly. But what exactly changes in the electron wave functions when an insulator becomes a metal?
Gravitational waves are not vibrations of matter, but tremors of spacetime itself, predicted by Albert Einstein. They travel at the speed of light and pass through objects, stretching and squeezing them.
A pebble tossed into a pond sends ripples spreading in all directions. Now imagine the pond itself suddenly turning into jelly — instantly, faster than the wave can complete a single crest. Some ripples would keep spreading but change their spacing, while others would unexpectedly turn around and run back toward the point of impact, as if time were flowing backward for them.
A hot spoon in a cup of tea — heat runs along the metal from the hot end to the cold one. Textbooks describe this process as atoms jiggling and passing on their jolts to each other. But atoms don't just jiggle: they also spin, like tiny tops. Until now, physicists had no common language to describe both motions at once.
The authors of the work built such a language.
Plutonium is a metal with attitude. One form shrinks when cooled, another swells. But at room temperature, the alloy behaves strangely: the ruler says one thing, X-rays say another. The ruler shows the sample barely grows, while X-rays see atoms in the crystal lattice moving further apart.
In a dark room, a flashlight beam picks out only a narrow strip from the gloom. In much the same way, Roger Penrose proposed looking at gravitational waves — ripples in spacetime traveling at the speed of light.
An ordinary crystal is like an apartment building: electrons move through shared hallways and staircases, influencing each other through the walls. Now, imagine removing all the walls, leaving just a single line of apartments. How would the residents behave?
Hydrogen has nothing to do with it, but the collective behavior of electrons takes center stage.
A pebble drops into a pond, and neat circles spread across the water. But the pond's bottom is strewn with invisible glass shards: each one slightly delays the wave, scatters it here, or alters its pace. That's roughly how gravitational waves, the trembling of space itself, pass through distant galaxies and dark clumps of matter.
When light knocks an electron out of an atom, it flies off like a ball thrown into a crowd. Scientists have long wanted to know the exact moment each electron leaves the atom, but direct measurement disturbed the very process. Now physicists have proposed a method that uses a second light pulse to 'photograph' the moment of the electron's birth.
A water molecule resembles a tiny dumbbell: two hydrogen atoms attach to an oxygen atom at an angle. This dumbbell doesn't stay still: it stretches, compresses, and rotates. Each such motion has its own energy, like steps on a ladder.
Light is not just a beam but a wave with an electric field that changes at a speed unimaginable to ordinary clocks. Until now, this field could only be measured at a single point, like taking temperature with a single thermometer. Now researchers have created a method that shows the entire field at once, like a thermal imager showing a heat map.
In the dark cloud L43, where stars are born, dust grains twirl like tiny compasses. Light from a young star pushes them, while the magnetic field lines them up in a specific direction. When a grain is turned sideways to us, its heat reaches us polarized, like light passing through a narrow slit.
A stone drops into a pond — ripples spread across the water. Do short waves outrun long ones? No, in deep water it's the opposite: long waves overtake short ones. In metal, sound of one pitch travels at one speed, another pitch at another.
The ocean is like a layered cake: warm, light water on top, cold, heavy water below. Between the layers, at the interface, invisible waves roam. They don't lift crests like a storm; instead, they slowly rock the entire water column, as if someone were shaking a giant aquarium from within.
A quantum system, once born, does not forget it. Even after dozens of lifetimes, a trace of the initial state remains in its decay: a slowly decreasing power-law tail. For two fluorescent dyes, erythrosine B and eosin Y, this tail has been observed for the first time in two spectral channels simultaneously.
A single photon passes through two slits and leaves an interference pattern on a screen. Quantum mechanics describes this process with a wave function, but what happens to the particle itself?
Two translators listen to the same symphony. One hears only the fundamental tone: a clean, predictable melody. The other catches the overtones that color every note.