quantity

coherence time

The time over which a wave's phase remains predictable, limiting interference visibility.
36 related articles

Description

Coherence time also plays a role in astrophysics and cosmology. For example, in the search for dark matter, certain proposed particles like axions are expected to produce coherent signals over long timescales. The article 'Солнечная гравитационная ловушка для ультралёгкой тёмной материи' (Solar gravitational trap for ultralight dark matter) discusses how the Sun's gravity could concentrate dark matter, potentially enhancing its coherence and making it detectable. In gravitational wave astronomy, the coherence of the signal is essential for extracting faint signals from noise, as explored in 'Как услышать шёпот гравитации, не потеряв ни слова' (How to hear the whisper of gravity without losing a word).

History

The concept of coherence time emerged from classical optics in the 19th century, with Thomas Young's double-slit experiment demonstrating interference. The formal treatment of coherence was developed by Emil Wolf and others in the 1950s, leading to the modern theory of optical coherence. In quantum mechanics, the idea of decoherence was formalized in the 1970s and 1980s by physicists like H. Dieter Zeh and Wojciech Zurek.

How it works

Coherence time is fundamentally limited by interactions with the environment. For a photon, scattering off atoms or fluctuations in the medium can randomize its phase. For a quantum bit (qubit), interactions with stray magnetic fields or thermal vibrations cause decoherence. The longer the coherence time, the more isolated the system is from its surroundings. Techniques to extend coherence time include cooling to near absolute zero, using materials with low noise, and employing dynamical decoupling—a sequence of pulses that reverses the effects of environmental noise. In interferometry, coherence time is related to the bandwidth of the source: a narrow-band source (like a laser) has a long coherence time, while a broadband source (like sunlight) has a very short one.

In practice

Coherence time is a key parameter in quantum computing, where it determines how long qubits can retain information before errors occur. It is also critical in optical coherence tomography (OCT), a medical imaging technique that uses low-coherence light to produce high-resolution cross-sectional images of biological tissues.

Fun fact

The coherence time of a typical atomic clock's microwave signal is so long that if you started a wave at the Big Bang, it would still be coherent today, having oscillated about 10^30 times without losing phase.

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Related articles · 36

HEP Phenomenology2026-08-062 minarXiv:2608.05538express
Dark Matter from Thermal Noise
In the first moments after the Big Bang, the universe resembled a boiling cauldron. According to one hypothesis, dark matter, the invisible substance that holds galaxies together, could have been born there.
HEP Phenomenology2026-08-052 minarXiv:2608.05082express
How Particles Are Born from the Void
The quantum world is like a kitchen where particles suddenly appear out of "nothing." But you need a chef — a classical field acting as an external source. Glauber's theorem, long known in optics, has now been generalized: it shows exactly how the field "cooks up" particles, be they photons or gravitons.
Cosmology2026-08-041 minarXiv:2608.03739express
The Universe's Memory of Gravitational Waves
A gravitational wave from a black hole merger is like a bell tolling in the night. The loudness tells you how far away the source is. But to learn how fast the night itself, the cosmos, is expanding, you usually need a second signal: a flash of light or a catalog of galaxies. Both are rare to catch.
General Relativity2026-07-312 minarXiv:2608.00281express
Two Signals in the Universe's Noise
A noisy café. You're trying to make out two quiet conversations: one from the table by the window (black hole mergers), the other a barely audible whisper from the far corner (echoes of the universe's birth). But the hiss of the espresso machine and street noise (detector jitter) drown everything out. New work teaches a computer to separate these sounds.
Cosmology2026-07-123 minarXiv:2607.10607
Cosmology2026-07-065 minarXiv:2607.05044
Symphony of Dark Energy: From Heavy Adagio to Explosive Allegro
A drama is brewing in cosmology: two principal musical instruments, the orchestra of the early Universe and the chamber ensemble of the modern cosmos, play the same symphony of expansion at different tempos.
Cosmology2026-07-052 minarXiv:2607.04460
Cosmic Metabolism: Dark Energy Feeds Matter
The standard model of cosmology, based on the field equations proposed by Einstein, describes the Universe as a cocktail of dark matter (discovered thanks to Vera Rubin) and dark energy in roughly a 1:3 ratio.
Cosmology2026-07-053 minarXiv:2607.04550
Cosmic Metronome: Binary Stars Search for Axion Dark Matter
In a close binary system, the hot star, like a searchlight, illuminates its cooler companion. Some of the light scatters off free electrons in its atmosphere — this is Thomson scattering — and acquires linear polarization. As the stars orbit each other, this polarization rotates, like the hand of a peculiar cosmic metronome.
General Relativity2026-06-261 minarXiv:2606.28161express
Gravitational atoms of axions sing in black hole pairs
A black hole, like a spinning wheel, twists a cloud of light particles, axions, around itself. These particles are the leading candidates for dark matter. The cloud follows the laws of quantum mechanics, resembling a giant atom: there are levels, and there are transitions between them.
HEP Experiment2026-06-221 minarXiv:2606.22814express
Levitating Magnet Catches Dark Matter
In the pitch darkness of a vacuum chamber, a tiny magnet floats. It touches no walls and loses almost no energy — an ideal sentinel, ready to catch the faintest nudge. Such a sentinel is exactly what you need for axion hunting. These particles are prime suspects in the case of the Universe's hidden mass, which we call dark matter.
General Relativity2026-06-222 minarXiv:2606.23418express
Dark Matter from Twisted Space
The early universe was a restless place. Space trembled with gravitational waves — ripples in the very fabric of reality. In this churning cauldron, dark matter is thought to have been born. But the newborn particles had no mass: it had to come from somewhere. Usually, the Higgs field is responsible for mass.
HEP Phenomenology2026-06-182 minarXiv:2606.20524express
Dark Matter from Black Holes with Axion Boost
In the early Universe, tiny black holes could have been born — mountain-mass but atomic-nucleus-sized. Today they could serve as factories for dark matter. There are two mechanisms: the familiar evaporation (Hawking radiation) and the lesser-known superradiance.
HEP Phenomenology2026-06-152 minarXiv:2606.16099express
Laser Interferometers as Detectors of Axion Dark Matter
The universe is permeated by invisible mass, dark matter, whose existence was first proposed by Fritz Zwicky in the 1930s, based on his observations of galaxies moving in clusters.
General Relativity2026-06-091 minarXiv:2606.10776express
Black Hole as a Gravitational Atom: Gravitational Echo
If a black hole spins quickly, it can hold a cloud of ultralight particles around it, so light that their mass almost vanishes. They arrange themselves in layers, like electrons in an atom, only here gravity does the job instead of electric forces. This structure stores energy, like a coiled spring.
General Relativity2026-06-021 minarXiv:2606.04099express
Weak Attraction: How Gravity Spares Quantum Superpositions
A single particle can be in two places at once — that's superposition. But any interaction, like a shout, instantly 'collapses' this uncertainty. It was long thought that even gravity could interfere.
General Relativity2026-05-301 minarXiv:2606.00577express
Gravitational Waves: Listening to Space without Templates
Astronomers listen to the cosmos like an old radio: they twist the knob not to find a particular station, but to catch any unusual noise. This approach breaks the mold: instead of hunting for gravitational waves using memorized patterns, they catch everything — without bias.
Cosmology2026-05-262 minarXiv:2605.27357express
Gravitational Sirens: Where to Find the Key to the Dark Universe
Two dots on the surface of a balloon: that's all the reference points you have when trying to figure out how it inflates. That's roughly how cosmologists reconstruct the history of the universe's expansion.
Cosmology2026-05-211 minarXiv:2605.22944express
Strings of the Cosmos: How to Catch the Universe's Tremors
A fundamental string plucked at the moment of the Big Bang doesn't just hum a single note — waves run along it, and occasionally tiny loops peel off. These loops, like tuning forks, begin to ring at their own frequency, producing a very high-pitched sound.
HEP Phenomenology2026-05-201 minarXiv:2605.21092express
Dark matter sings in magnetic fields
In the first moments after the Big Bang, the universe was a boiling cauldron. But then, according to a new hypothesis, it suddenly cooled dramatically — far more than previously thought. In this icy world, dark matter particles, like tiny pendulums, froze and did not begin their oscillations.
Cosmology2026-05-151 minarXiv:2605.16155express
Dark Dialogue: Gravitational Lenses Reveal an Exchange of Matter and Energy
The Universe is a vast city. In it, dark matter is the invisible framework of buildings, and dark energy is the force stretching the streets. For a long time they were considered independent, but new research has caught them in secret communication.
HEP Phenomenology2026-05-111 minarXiv:2605.11078express
A Trap for Dark Matter Particles
Dark matter has eluded direct observation so far, even though its gravity holds galaxies together. One hypothesis: it’s made of axions — ultra-light particles predicted by theory.
Mesoscale2026-05-102 minarXiv:2605.09488express
Dark Excitons: A Quantum Trickle in a Chip
In a thin sandwich of semiconductors, light creates pairs, an electron and a positive hole, that stick together like a ball on a rubber band. Normally, such pairs, called excitons, quickly emit light and vanish. But there are others, dark ones, that live hundreds of times longer because their internal structure forbids them from easily giving off energy.
Cosmology2026-05-071 minarXiv:2605.05906express
Dark Matter Speaks in Radio Waves
Dark matter is invisible, but its gravity governs the motion of galaxies. What it's made of is a mystery. One idea: it consists of ultra-light particles akin to axions.
HEP Phenomenology2026-04-292 minarXiv:2604.26860express
Why Gravitational Waves Whisper About a Hundred Mega-Electronvolts
In a vast hall, a hundred tuning forks are set out. Each one is a pulsar — an ultra-dense stellar remnant spinning at a furious rate, sending out radio pulses more precisely than any clock. When a low-frequency sound wave sweeps through the hall, all the tuning forks start to go slightly out of tune at the same moment.
HEP Phenomenology2026-04-241 minarXiv:2604.22336express
The Quantum Pond: How an Ion Crystal Catches Dark Matter
A flat crystal of charged atoms suspended in an electromagnetic trap behaves like a perfectly calm pond. The slightest breeze, and ripples spread across its surface. This 'pond' catches the splashes from dark matter particles and the ripples of spacetime — high-frequency gravitational waves.
High Energy2026-04-223 minarXiv:2604.21010express
Gravitational Echoes from Distant Black Holes
When two supermassive black holes circle each other before merging, they shake spacetime itself, like a speedboat racing across a lake leaves waves in its wake. These waves are called gravitational waves. They travel through the Universe and pass through everything, even the Earth.
HEP Phenomenology2026-04-162 minarXiv:2604.15241express
Threads Left from the Very Beginning
In the first moments after the Big Bang, the cosmos resembled a giant cooling pond. Just as water, when freezing, becomes covered with a network of cracks, so the cooling universe could have cracked — not into ice, but into the thinnest filaments of pure energy. These filaments are called cosmic strings.
HEP Phenomenology2026-03-231 minarXiv:2603.22647express
Levitating Magnet Catches Dark Matter
A tiny superconductor, levitating above a magnet, is like a cork on the surface of an invisible ocean. The slightest breath of dark matter makes it shudder. Scientists examined two kinds of such 'wind'. The first – gravitational waves, which stretch and squeeze space itself, like ripples on the fabric of the cosmos.
HEP Phenomenology2026-03-101 minarXiv:2603.10189express
A Pulsar as a Beacon for Invisible Particles
A neutron star the size of a city spins thirty times per second. Its magnetic field is trillions of times stronger than Earth's. Such conditions could spawn a cloud of axions around the star — light particles that no detector has caught yet, but which neatly explain the hidden mass of the Universe.
Quantum Physics2026-02-202 minarXiv:2602.18147express
Synchronizing Clocks with Weak Light
Two clocks in different rooms need to tick in unison. Usually, this is done by sending bright pulses or pairs of photons that arrive one right after the other. But the signal can be so weak that photons barely make it through. In this work, clocks were synchronized with light a billion times dimmer than usual.
HEP Phenomenology2026-02-061 minarXiv:2602.06922express
Cosmic Seesaw: How the Young Universe's Pulsations Boosted Dark Matter
In its infancy, the universe was a hot, plasma-like mixture of particles. Microseconds after the Big Bang, as it cooled, the temperature fluctuated slightly.
HEP Experiment2026-01-282 minarXiv:2601.21074express
A Trap for the Invisible: An Array of Resonators
A pot on the stove rings when the water boils. An empty copper cup can also "ring"—at radio frequencies — if a dark matter particle is born inside it. These particles are called axions, and according to one hypothesis, they fill the entire galaxy as an invisible cloud.
HEP Phenomenology2026-01-081 minarXiv:2601.04576express
A Trap for Invisible Axions: A Magnetic Detector
Dark matter is five times more massive than ordinary matter, yet it emits no light. Its nature remains unknown. One candidate is the ultra-light axion particle. Axions could pierce right through the planet, barely noticing atoms.
General Relativity2026-01-051 minarXiv:2601.02197express
A Black Hole Like a Bell: How a Light Pulse Gives Rise to Echoes
If you briefly flash light near a black hole, it will respond with a long echo, like a bell that keeps ringing after being struck. The light gets trapped near the hole, bouncing repeatedly off an invisible boundary: the photon sphere, where rays circle around like sound in a metal.
HEP Phenomenology2026-01-021 minarXiv:2601.00955express
A Solar Trap for Dark Matter
The Sun’s gravity creates an invisible goblet, in which dark matter of a special kind — ultralight — doesn’t splash around chaotically, but occupies strict energy steps, like transparent layers of liquid. So around the Sun, a natural spectroscope emerges, sorting the invisible substance into levels, just like electrons in an atom.
A Ruler Made of Light: Measuring Picoseconds with Frequency Resolution
A ruler made of light: that's one way to describe a new method for measuring tiny time delays. In 1987, Chong Ki Hong, Zhe-Yu Ou, and Leonard Mandel noticed that when two indistinguishable photons hit a beam splitter simultaneously, they always exit together from the same port.