object

ultralight axion

A hypothetical very light particle that could explain certain cosmological observations, such as CMB polarization rotation.
19 related articles

Description

An ultralight axion is a hypothetical elementary particle with a mass far smaller than that of an electron, often in the range of 10^-22 to 10^-10 eV/c². It is a leading candidate for dark matter, the invisible substance that makes up about 27% of the universe. Ultralight axions are predicted to have a very long de Broglie wavelength, meaning they behave more like waves than particles on galactic scales, potentially explaining certain cosmological observations such as the rotation of the polarization plane of cosmic microwave background (CMB) radiation.

History

The axion was first proposed in 1977 by Roberto Peccei and Helen Quinn to solve the strong CP problem in particle physics, and later realized to be a dark matter candidate. The idea of ultralight axions (also called fuzzy dark matter) was developed in the 2000s by Wayne Hu, Rennan Barkana, and Andrei Gruzinov.

How it works

Axions interact with photons through a coupling that causes the polarization of light to rotate as it travels through an axion background. This effect, known as cosmic birefringence, would leave a distinct signature in the CMB polarization pattern. The axion field oscillates coherently, and its interaction with electromagnetic fields is described by a term in the Lagrangian that couples the axion field to the electromagnetic field tensor. The rotation angle depends on the axion mass and coupling strength, allowing observations to constrain these parameters.

In practice

Currently used in experimental searches for dark matter, such as the Axion Dark Matter Experiment (ADMX), which looks for axion-photon conversion in a microwave cavity.

Fun fact

If ultralight axions exist, they would form a coherent wave that could create interference patterns in the Milky Way's dark matter halo, potentially detectable as tiny oscillations in pulsar timing.

Concept graph →

Related articles · 19

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HEP Phenomenology2026-07-311 minarXiv:2607.29492express
Dark Matter from Magnetic Droplets
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Cosmology2026-07-222 minarXiv:2607.20614
HEP Theory2026-07-082 minarXiv:2607.07295express
Dark Matter from Five Dimensions
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Cosmology2026-06-101 minarXiv:2606.12521express
Dark Matter Decays and Slows the Universe's Growth
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Cosmology2026-06-082 minarXiv:2606.09994express
The Cosmos Twists Light
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Cosmology2026-06-042 minarXiv:2606.06410express
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General Relativity2026-05-171 minarXiv:2605.17589express
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The universe is full of invisible substance that governs the movement of galaxies. In the 1970s, astronomer Vera Rubin showed: without dark matter, stars on the outskirts would have long since flown apart. But what it's made of remains unknown.
HEP Phenomenology2026-05-072 minarXiv:2605.06777express
Dark Matter Changes the Face of Neutrinos
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The Cosmic Loom: The Puzzle of Missing Antimatter and Inflation
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HEP Phenomenology2026-04-302 minarXiv:2605.00103express
Axion Stars: Gravitational Clumps of Dark Matter
Axions are hypothetical elementary particles introduced in 1977 by Roberto Peccei and Helen Quinn to resolve the so-called strong CP problem in the Standard Model of particle physics.
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Hunting an Invisible Particle in Kaon Decays
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High Energy2026-03-121 minarXiv:2603.11922express
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High Energy2026-02-051 minarXiv:2602.06192express
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The night sky is full of beacons, but some shine in a way that makes them nearly invisible. Astronomers have discovered a new class of objects: ultrasoft X-ray sources. They are so "cool" by X-ray standards that their emission falls at the boundary between ultraviolet and soft X-rays, where ordinary telescopes are almost blind.
HEP Phenomenology2026-01-131 minarXiv:2601.08567express
Ghost Particle: How Scientists Caught a Hint of a New Force
At Hungary's Institute for Nuclear Research, ATOMKI, physicists noticed something odd: in the decays of excited atomic nuclei, pairs of electrons and positrons sometimes fly apart at an unusual angle. It's as if an invisible mediator particle briefly appears and disappears between them.
Cosmology2026-01-011 minarXiv:2601.00443express
Dark Matter Gave Rise to Galactic Magnetic Fields
Without the invisible framework of dark matter, galaxies would fly apart. Astronomer Vera Rubin proved back in the 1970s that stars rotate as if held by an unseen mass. But new research shows it's not just passive ballast.
Cosmology2025-10-081 minarXiv:2510.07382express
Invisible Object Weighing a Million Suns: Gravity Acts as a Magnifying Glass
Astronomers have found an invisible object in the Universe weighing just a million Suns — for cosmic scales, that’s a mere trifle, a hundred times lighter than anything they’ve been able to “weigh” at such distances. The object itself doesn’t shine, but it gave itself away by bending the light from an even more distant galaxy.
High Energy2025-10-071 minarXiv:2510.06193express
Sky Hotspots: The Senders of Ultra-Particles Identified
Every day, particles with colossal energy enter Earth's atmosphere, like unsigned letters. Their source long remained a mystery. New research shows: these 'visitors' point to nearby galaxies, where from time to time catastrophes occur — collisions of neutron stars, ultra-dense spheres the size of a city but with the mass of the Sun.