Earth as a Dark Matter Detector ✛ ✎

Original: "Searching for dark photon dark matter from terrestrial magnetic fields"
arXiv:2509.15783 · 2025-09-19 · arXiv non-exclusive · independent analysis · 1 min
Earth's magnetic field helps search for elusive dark photons.

Invisible dark matter governs the rotation of galaxies — Vera Rubin showed back in the last century that stars move as if pushed by an unseen force. One of the prime suspects is the dark photon, a massive cousin of ordinary light, predicted by the extended equations of Maxwell and not fitting into the Standard Model.

Scientists turned the planet into a giant radio receiver. The space between Earth and the ionosphere (the electrically charged layer of the atmosphere) forms a resonator that greatly amplifies magnetic tremors if their frequency matches the 'radio wave' of a dark photon. It's like one guitar string resonating to a note played on another. Years-long magnetic field records enabled a delicate spectral analysis — fishing out a single frequency from the noise.

For the first time, air conductivity was taken into account, refining the calculation and helping to separate a possible signal from interference. They didn't hear a direct 'hello' from dark matter, but they set the strictest limits on its interaction with magnetism — for a mass range from 10⁻¹⁵ to 2×10⁻¹³ eV. And the sought frequencies below 100 Hz, where whales sing and power lines hum, force scientists to scrub the sounds of the ocean and civilization from the data.

The sought signal lies in the band below 100 Hz — here whales sing and power grids hum. To catch the cosmic 'whisper,' scientists have to filter out the voice of the ocean and the noise of civilization.

f_{A'} = \frac{m_{A'}}{2\pi}
The oscillation frequency of the field equals the particle mass divided by 2π (in natural units).
\varepsilon \lesssim 5\times 10^{-11}
At a mass of 3×10⁻¹⁴ eV, the mixing parameter does not exceed 5×10⁻¹¹ with 95% confidence.
Scientists
Fritz ZwickyArthur ComptonMichael FaradayHendrik LorentzVera RubinCharles Townes
Concepts
dark photon dark matter resonance microwave photon direct detection experiments dysprosium magnetic domain imaging magnetophotonic effects magnetic field mass range millivolt per meter axion detector photomultiplier tube resonant cavity gamma ray spectroscopy light matter coupling astrochemical spectroscopy cosmic dust magnetism black hole shadow anomalies magnetometer rare event search