object

cosmic string

A topological defect in spacetime that may form without a singularity.
39 related articles · 1 formulas

Description

Cosmic strings are hypothetical one-dimensional topological defects in the fabric of spacetime, predicted by many particle physics theories. Unlike black holes, they are not formed by gravitational collapse but are thought to have been created during phase transitions in the early universe, when the symmetry of the fundamental forces broke in different ways in adjacent regions. They are extremely thin—far thinner than a proton—but can be enormously long, potentially stretching across the observable universe, and carry immense energy density.

History

The concept was first proposed by Tom Kibble in 1976, building on the idea of topological defects in quantum field theory. The term 'cosmic string' was coined shortly after by Alexander Vilenkin and others who developed their cosmological implications.

How it works

As the early universe cooled, it underwent phase transitions similar to water freezing into ice. When different regions settled into different 'orientations' of the broken symmetry, the boundaries between them could form stable, thread-like structures. These strings are topologically stable because they cannot be broken without creating a free end, which is forbidden by the underlying physics. Their immense mass per unit length warps spacetime around them, causing light passing by to be gravitationally lensed, and they would emit gravitational waves as they oscillate and interact.

In practice

Cosmic strings are primarily of theoretical interest, but their detection would provide direct evidence for high-energy physics beyond the Standard Model. They are also studied as potential sources of gravitational waves that could be observed by detectors like LIGO and pulsar timing arrays.

Fun fact

If a cosmic string passed through Earth, it would be virtually undetectable directly, but it would cause a tiny, instantaneous jump in the planet's rotation speed due to the distortion of spacetime.

Concept graph →

Formulas

$$G\mu = \frac{\mu}{m_{\text{Pl}}^2}$$
Dimensionless measure of cosmic string energy density.
What is in the formula
μvariablemass per unit length of cosmic string — linear mass density kilogram per metre
GconstantNewton's constant of universal gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
m_PlconstantPlanck mass, the fundamental mass scale in quantum gravity — planck mass = 2.176434e-8 kilogram
gμ=\frac{μ}{m_{{pl}}^2} · 2607.20340v1

Related articles · 39

Cosmology2026-07-282 minarXiv:2607.25317express
Current-Carrying Cosmic Strings and Their Gravitational Imprint
Right after the Big Bang, space cooled unevenly. In some places, folds could have formed — threads of energy as thin as a hair but incredibly dense. Physicists call them cosmic strings. They oscillate, collide, and emit gravitational waves — ripples in the fabric of space itself.
HEP Theory2026-07-282 minarXiv:2607.26124express
Cosmic Strings: Echoes of the Universe's Birth
In the first fractions of a second after the Big Bang, the universe was a stage of rapid change. A stretched rubber sheet that cools quickly becomes covered with microscopic cracks. A similar process on a cosmic scale could have given rise to cosmic strings — ultra-thin but super-dense threads of energy stretching across the entire universe. These strings are not just defects in space.
When the Universe Freezes: Gravitational Waves from Cosmic Strings
The early Universe was like a rapidly cooling ocean. At colossal temperatures, everything was one — quarks, electrons, forces all blended into a symmetric 'steam.' But as it expanded and cooled, this steam condensed, phase transitions cascading one after another like water turning to ice.
HEP Theory2026-07-172 minarXiv:2607.16120express
The String That Refuses to Go Quiet
Pluck a guitar string, and it will vibrate and quickly fade. Now imagine a cosmic string: an ultra-thin filament of pure energy left over from the Big Bang, trillions of times thinner than an atom and denser than a neutron star. Strike it, and it might sing for billions of years.
math.GN2026-07-013 minarXiv:2607.01068
The Sieve of Infinity: How Q-spaces Intertwine with Measurable Cardinals
In mathematics there is a sieve that sifts not dust, but infinity itself. It’s called a Q-space: here any subset turns out to be a Gδ set — a countable intersection of open sets, as if sifted through an unimaginably fine mesh.
General Relativity2026-06-282 minarXiv:2607.00036express
Tubes Instead of Points: How Matter Sidesteps Einstein's Ban
An object cannot be a point. At least, not in Einstein's gravity. The equations of general relativity require that the source of the field, matter, be smeared out in space, not concentrated in an infinitesimal volume. Otherwise, infinities appear in the formulas, and a smooth spacetime cannot be constructed.
HEP Phenomenology2026-06-232 minarXiv:2606.25014express
Dark Matter from Bubbles
The hot broth of the early universe cooled unevenly. At some point, bubbles of a new phase began to pop within it, like steam bubbles in boiling water. But these bubbles weren't made of steam; they were made of a new state of matter in which particles of the dark sector clumped into larger lumps. That's how dark matter could have been born.
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.
General Relativity2026-06-222 minarXiv:2606.23846express
Black Holes from the Universe's Infancy
It all began not with emptiness, but with a boiling ocean of plasma. In that primordial broth, sound waves raced through the fiery matter, colliding and compressing it. Sometimes a clump grew so dense that light could no longer escape, and right out of the scorching gas, a primordial black hole was born.
HEP Phenomenology2026-06-182 minarXiv:2606.20524express
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General Relativity2026-06-182 minarXiv:2606.20540express
Gravity Doesn't Always Respect Cosmic Censorship
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HEP Theory2026-06-181 minarXiv:2606.20942express
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The Universe behaves like a soap bubble swelling in a multidimensional foam. The dark bubble model explains why it's expanding ever faster: the spacetime bubble grows, and its membrane gains a tiny thickness — about a micron, like a bacterium. At such distances, gravity 'blurs' across this thickness and weakens.
General Relativity2026-06-122 minarXiv:2606.14815express
Quantum Corrections to a Black Hole in a Dark Web
A black hole is not just a cosmic vacuum cleaner. It is a region with such strong gravity that even light cannot escape it. But place it in a perfect fluid of dark matter and add a cloud of strings, thin filaments stretched across all of space, and the picture gets more complicated.
The Snapping Cable of Reality: How Finite String Thickness Accelerates Quantum Decay and Reshapes the Gravitational Hum
Immediately after the Big Bang, in the seething cauldron of the cooling Universe, much like in unevenly hardening glass, stresses appeared — hairline cracks in reality, cosmic strings. Picture a tightrope walker balancing on an invisible cable stretched across the abyss of warped spacetime.
Cosmology2026-05-211 minarXiv:2605.22944express
Strings of the Cosmos: How to Catch the Universe's Tremors
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Disordered Systems2026-05-142 minarXiv:2605.14349express
Disorder That Doesn't Destroy Everything
A crystal is like a row of soldiers on a parade ground: every atom is in its place, and electrons march through it in neat waves. An amorphous material is like a crowd at a train station, where there is no order, just a jostling throng. In such a crowd, an electron usually gets stuck quickly, like a person trying to push through a dense mass of people.
Cosmology2026-05-143 minarXiv:2605.15197
Invisible Drums: How Gravitational Waves Give Birth to Black Holes
The mystery of dark matter, first glimpsed in the stellar whirlpools by Vera Rubin, has been tormenting physics for nearly a century. One of the boldest hypotheses: primordial black holes, born in the scalding broth of the early universe.
Cosmology2026-05-111 minarXiv:2605.10476express
Dark Energy Isn't Constant?
For a long time, dark energy, the mysterious force prodding the expansion of the Universe, was considered eternal and unchanging, like yeast that never loses its activity. But explaining such constancy through the laws of the microcosm proved impossible, and scientists began to suspect that the “leaven” might be going flat.
General Relativity2026-05-102 minarXiv:2605.09786express
How Gravity Loops the Invisible
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HEP Theory2026-05-062 minarXiv:2605.05336express
Wormholes Set Limits on Imagination
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HEP Phenomenology2026-05-042 minarXiv:2605.03003express
Cosmic Strings That Melt
When hot soup cools, clumps form on the surface — similarly, as the early universe cooled, it gave birth to threadlike clumps of energy: cosmic strings. Some of them are like a stretched rubber band: as long as it's intact, it's stable. But if you nick the band, it snaps.
HEP Phenomenology2026-04-292 minarXiv:2604.26191express
A Cosmic Bubble with a Monopole Inside
A magnet with only one pole (north, without a south) is not a fragment but a particle in its own right. Physicists call it a magnetic monopole (a carrier of a single magnetic charge). Such visitors could have been born in the early universe, when the forces were just separating.
HEP Phenomenology2026-04-281 minarXiv:2604.26005express
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Cosmology2026-04-231 minarXiv:2604.21520express
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General Relativity2026-04-221 minarXiv:2604.20656express
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HEP Phenomenology2026-04-162 minarXiv:2604.15241express
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HEP Experiment2026-04-121 minarXiv:2604.10732express
Hunting for Microscopic Black Holes
From 2016 to 2018, at the Large Hadron Collider at CERN, protons collided at energies of 13 teraelectronvolts, as if two peas were accelerated to speeds where their impact spawns a whole swarm of new particles.
Cosmology2026-04-021 minarXiv:2604.02300express
Weighing Neutrinos by the Cosmic Web
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HEP Phenomenology2026-04-011 minarXiv:2604.01304express
Little Red Dots and Giant Black Holes
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General Relativity2026-03-221 minarXiv:2603.21187express
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Cosmology2026-03-051 minarXiv:2603.05191express
Gravitational echo saves the Universe from excess black holes
The Big Bang was like a cosmic thunderclap that set the fabric of space vibrating. These vibrations — gravitational waves — still echo through the Universe like a fading rumble from that ancient event. The louder the initial 'bang,' the more primordial black holes should have formed.
HEP Phenomenology2026-03-031 minarXiv:2603.02996express
Monopoles on Strings: A New Source of Gravitational Waves
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General Relativity2026-02-121 minarXiv:2602.12101express
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