ghost

A campfire burns steadily and long. But when the wind blows, the flame flickers out, leaving only embers. A similar story plays out with the gravastar — a hypothetical object that was supposed to replace the black hole. An ordinary black hole hides a singularity — a point where the laws of physics break down.

In the first moments of the universe's life, there was not even a hint of dark energy — the very force that today pushes galaxies apart ever faster. But if you look deeper, down to the Planck scale (billions upon billions of times smaller than an atomic nucleus), spacetime ceases to be smooth.

The explosion of a distant supernova told us something hard to believe: the universe is expanding faster and faster. The engine of this acceleration is dark energy — nearly 70% of everything that exists.

A ball sits in a pit. It won't roll out on its own: it needs a push. But in the quantum world, a particle can leak through a barrier without extra energy. This trick is called tunneling.

In the late 1990s, astronomers including Saul Perlmutter discovered that the universe is expanding at an accelerating rate. The cause was dubbed dark energy — an invisible force stretching the cosmos.

An inflating balloon starts out slowly, then suddenly expands faster and faster, as if someone is pumping it up from inside. That's roughly how our universe behaves: galaxies are receding with acceleration. The culprit behind this acceleration is called dark energy.

Back in the 1930s, Fritz Zwicky noticed that the speeds of galaxies in clusters were too high for the visible mass. Later, Vera Rubin confirmed this for individual galaxies.

A ball on a slope with two pits usually rolls into the nearest one and comes to rest. But if the slope is slightly deformed and 'remembers' recent nudges, the ball can hang around halfway for a long time — in a narrow spot it doesn't want to leave. That's exactly the trick physicists played with light.

Spacetime sometimes resembles a sheet of paper in which you can punch a hole and connect the edges with a short tube: you get a wormhole. In the simplest mathematical models of such wormholes, massless scalar fields appear — something like an invisible fog filling everything around.

Sometimes an unwelcome guest sneaks into the equations, like a creaky floorboard that unsettles the whole house. In gravity theories, if you add curvature-squared terms to the equations (which you need to describe very strong fields), a ghost particle appears — heavy but with negative energy.

In 2015, the LIGO detectors caught the first burst of gravitational waves — astronomers heard two black holes colliding far out in space. That ripple in spacetime reached us with its signal shape intact: like the sound of a bell traveling billions of years without distortion.

A drummer stays silent, but from the pauses you can tell where he didn’t hit. Similarly, physicists built an image by catching not light, but moments of absolute darkness. The picture emerged from silence. In the experiment, they shone light from an ordinary lamp onto the object.

When two black holes collide, they send out gravitational waves and ring like a massive bell. The fading sound, or ringdown, carries the imprint of the final black hole. But if dark energy, the force accelerating the universe, changes over time, it can cling to the black hole like a thin paint layer.

An attempt to suppress room background noise by adding anti-sound turns into speaker howl if the circuit has an error. A similar glitch occurred with a theory that set out to remove the main cosmic hum — the inexplicably weak dark energy.

When two black holes merge, the newborn hole should ring like a bell, emitting gravitational waves — ripples in space. Yet before the ring, a silence can fall: the black hole gets caught in a phantom trap, as if an invisible hand grips the bell’s clapper.