substance

x ray photon

A quantum of X-ray electromagnetic radiation, carrying energy and momentum.
21 related articles

Description

An X-ray photon is a quantum of electromagnetic radiation in the X-ray portion of the spectrum, with energies typically ranging from about 100 electronvolts (eV) to several hundred kiloelectronvolts (keV). Like all photons, it is massless, travels at the speed of light, and carries both energy and momentum, but its high energy gives it the ability to penetrate matter and interact with inner-shell electrons of atoms. X-ray photons are produced by transitions of electrons between deep atomic energy levels, by deceleration of charged particles (bremsstrahlung), or by synchrotron radiation from relativistic electrons in magnetic fields.

History

X-rays were discovered by Wilhelm Röntgen in 1895, but their nature as photons was established later. The concept of the photon itself was introduced by Albert Einstein in 1905, and the specific quantum nature of X-rays was confirmed through experiments on X-ray scattering by Arthur Compton in 1923, which demonstrated that X-rays behave as particles with momentum.

How it works

X-ray photons interact with matter primarily through three processes: the photoelectric effect, where the photon is absorbed and ejects an inner-shell electron; Compton scattering, where the photon scatters off an electron, losing energy and changing direction; and pair production, which occurs at very high energies (>1.022 MeV) near a nucleus, where the photon converts into an electron-positron pair. The energy of an X-ray photon is directly proportional to its frequency (E = hν, where h is Planck's constant), and its momentum is p = h/λ, where λ is the wavelength. These properties make X-ray photons a powerful probe of atomic structure and dynamics.

In practice

X-ray photons are used in medical imaging (radiography and CT scans), crystallography to determine molecular structures, and in X-ray astronomy to study high-energy phenomena in the universe.

Fun fact

The momentum of an X-ray photon, though small, is enough to measurably push atoms—this effect is used in techniques like X-ray photon correlation spectroscopy to study atomic motion.

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Related articles · 21

Plasma Physics2026-08-182 minarXiv:2608.17555express
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Quantum Physics2026-08-162 minarXiv:2608.15859express
Dim light kicks electrons out differently
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HEP Theory2026-08-042 minarXiv:2608.03747express
When Particles Whisper Goodbye
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Plasma Physics2026-08-021 minarXiv:2608.01323express
How the Electron's Shape Controls Gamma Light
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Cosmology2026-07-152 minarXiv:2607.14276
Photon Fog Forging Antimatter
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HEP Theory2026-06-102 minarXiv:2606.12513express
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Mesoscale2026-06-031 minarXiv:2606.04341express
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General Relativity2026-05-251 minarXiv:2605.25709express
When Black Holes Turn Inside Out
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Nuclear Theory2026-04-271 minarXiv:2604.24045express
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HEP Phenomenology2026-04-142 minarXiv:2604.13181express
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HEP Phenomenology2026-04-011 minarXiv:2604.01277express
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High Energy2026-03-291 minarXiv:2603.27805express
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physics.acc-ph2026-03-161 minarXiv:2603.15996express
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A typical accelerator is like an assembly line where electrons are the workpieces. To get the desired X-ray pulse, the workpiece is fine-tuned after it's already on the line: squeezed, filtered, corrected. In the new work, engineers decided to take a different approach — shaping the workpiece before it even hits the conveyor. At LCLS-II, electrons are knocked out of a metal by a short laser pulse.
HEP Phenomenology2026-03-071 minarXiv:2603.07010express
Stellar2026-02-012 minarXiv:2602.01323express
The Solar Flare Mystery: Light That Shouldn't Have Been There
A solar flare is like an explosion in the atmosphere: bright, fast, with different 'voices.' X-rays come from electrons that have been accelerated and then abruptly slowed down, losing energy. But in 2017, detectors on the Fermi satellite caught a different signal — gamma rays that didn't fit this picture.
Quantum Physics2026-01-121 minarXiv:2601.07694express
X-ray photons find each other
In a dark room, two flashlights shine on a wall. Usually, their beams simply add up, and the spot becomes brighter. But if the flashlights emit light in special packets, photons, then under certain conditions they can behave differently. Instead of independently hitting different spots, two photons 'agree' and only come out together, as a pair, from a single output.
General Relativity2026-01-071 minarXiv:2601.04145express
Invisible Vortices Sculpt Supermassive Black Holes
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Cosmology2025-11-182 minarXiv:2511.14163express
Light Gets Even Lighter: New Upper Limit on Photon Mass
Fast radio bursts are brilliant cosmic flashes that, like a starting signal, set off a race of radio waves across the universe. Astronomers used them as a natural laboratory to test whether the photon, the quantum of light and the carrier particle of the electromagnetic interaction, has mass.
Cosmology2025-09-112 minarXiv:2509.09472
Dark Matter Tuning Fork: How Axions Tune the Radio Sky
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