Dark Weather over Gran Sasso: Daily Rhythm of Sub-GeV Dark Matter ✛

Original: "Dark Matter Weather: Probing Sub-GeV Interactions with Earth-Shielding Modulation"
arXiv:2607.20620v1 · 2026-07-22 · CC BY 4.0 · 2 min
Daily oscillations in the flux of dark matter scattered within Earth's interior make it possible to distinguish its interactions with electrons and nuclei, and thus bring us closer to unraveling the nature of the lightest dark matter candidates.

At nine in the morning, the DarkSide-50 detector, 1400 meters beneath Gran Sasso, records a weak ionization pulse. By eleven at night, the frequency of such events drops noticeably. This is not an electronics glitch or a seasonal background variation.

Every day, the flux of dark matter reaching the detector changes by almost a factor of two in amplitude. The reason is Earth itself, which for some particles becomes almost transparent and for others an impenetrable screen.

This is how 'dark weather' manifests — a daily modulation caused by the scattering of dark matter particles inside the planet. A galactic wind of particles with masses tens of times smaller than a proton streams through the Solar System. Nothing like this exists in the Standard Model. As particles fly through Earth, they collide with nuclei. They lose energy. They change trajectory. For an underground detector, morning particles arrive almost directly, having passed through only a few hundred kilometers of rock. In the evening, the path lengthens to the full diameter of the planet—12 700 km. The flux weakens. Such a filter encodes information about the probability of nuclear scattering (cross section $σ_{SI}$_χn), while the detection itself in an argon target relies on ionization — interaction with electrons (cross section $σ_e$).

In the model with a dark photon, a hypothetical mediator mixed with the ordinary electromagnetic field, the cross sections on electrons and protons are tightly linked. It's like having a thermometer and barometer in one instrument: measuring one lets you predict the other. Deviations would signal more complex physics.

Numerical simulation (the DaMaSCUS package for Monte Carlo calculations) reproduced the distorted velocity distributions for different isoangles — angles between the detector and the galactic wind. The shape of the daily distribution is sensitive to the nuclear cross section. Analysis of DarkSide-50 data without time stamps gave an upper limit $σ_{SI}$_χn < 10⁻³³ cm² for masses 20–100 MeV. This is comparable to the best world constraints. Future detectors XENONnT and LZ with multi-year exposure will improve sensitivity by an order of magnitude. A network of setups in different hemispheres, like weather stations, will track phase and amplitude, confirming the reality of the signal.

Dark weather is not just a metaphor. It's a way to read the properties of invisible matter. Earth itself runs the experiment every day. Changing its perspective, it modulates the flux. And one day, the morning signal will tell us not only about the 'weather' underground, but about the fundamental laws of the Universe.

Over a day, the Gran Sasso detector (Italy) 'sees' dark matter traveling through up to 1300 km of rock; at night, when the detector faces away from the galactic wind, the path lengthens to nearly Earth's diameter—12 700 km. The flux reduction can differ by tens of percent.

The idea of planetary shadowing echoes the 'dark forest' concept from Liu Cixin's trilogy: civilizations hide, fearing discovery. Except here, Earth isn't hiding: it's helping us spot the hidden matter.

f(v) = \frac{1}{N} \exp\left(-\frac{v^2}{2\sigma_v^2}\right) \Theta(v_{\rm esc} - v)
probability to find a particle with a given speed
\frac{\sigma_{\chi e}}{\sigma_{\chi p}} \approx \left(\frac{\mu_{\chi e}}{\mu_{\chi p}}\right)^2
tight predictive link between electron and nuclear channels
Scientists
Paul DiracFritz ZwickyVera RubinMarie CurieEnrico FermiRoberto D. Peccei
Concepts
direct detection experiments dark matter indirect detection light matter interaction spectroscopy neutrino geophysics neutron scattering lz rare event search liquid xenon dune xenonnt semiconductor light interaction neutrino detector liquid argon gamma ray interactions manganese radiation detector neural network galaxy mapping subsurface ocean neutron diffraction borexino