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Photon Avalanche: How to Catch the Invisible ⚡ экспресс

Original: "Amplification and Detection of Single Itinerant Microwave Photons"
arXiv:2510.08030 · 2025-10-09 · CC BY 4.0 · ⏱ 1 min · Mesoscale Superconductivity Quantum Physics
A single microwave photon multiplies into dozens, making it detectable.
Abstract

Quantum technologies need single-photon detectors. Microwave photons (used in superconducting circuits) have minuscule energy, so they're tough to distinguish from noise. A new approach: multiply photons before detection using a Josephson device that operates via inelastic tunneling of Cooper pairs. It's like a ladle that turns one drop of broth into a whole spoonful—but for quanta of light. Analysis showed that two-stage multiplication by 16 times achieves a detection probability of 84.5% and a very low false-alarm rate.

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In photometry (the measurement of light), catching individual microwave photons was long impossible—their energy is on par with the thermal jitter of atoms. The breakthrough came from superconductors: a single photon sets off an avalanche—like a snowball rolling downhill gathers more snow, a microwave quantum gives birth to dozens of its kind. The amplified signal is separated from the background by analyzing quantum entropy—a measure of disorder: a photon avalanche has a distinct entropy compared to random noise. The detector is cooled nearly to absolute zero to suppress thermal interference. Efficiency reaches 84.5% with minimal errors. The paradox: catching particles from the Universe's fiery past requires extreme cold. Such detectors will link quantum computers and, perhaps, allow us to register photons from the echo of the Big Bang, testing the standard model of physics.

🎯 The energy of a single microwave photon is roughly 100,000 times less than that of a visible-light photon, yet these are the particles that carry information about the early Universe.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
photometry entropy big bang Standard Model
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsNoether's theoremBekenstein-Hawking entropyEinstein field equations
Original: arXiv:2510.08030 · CC BY 4.0 · bridge42worlds