Who nudged the atom in the detector? ✛

Original: "Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event"
arXiv:2609.01583v1 · 2026-09-01 · CC BY 4.0 · 1 min
A rare event in the LZ detector could be the trace of a dark matter particle, the higgsino.

Underground, there is a large tank filled with liquid xenon. One day, one of the atomic nuclei in this tank received a weak kick and recoiled, like a billiard ball struck by an invisible ball. The LUX-ZEPLIN detector recorded this kick, but scientists could not figure out what caused it. All the usual culprits, cosmic rays, radioactivity, did not fit.

Then an idea emerged: maybe it was a dark matter particle. Dark matter is invisible stuff that does not shine and barely interacts with ordinary matter, yet its gravity holds galaxies together. One possible dark matter particle is called the higgsino. It is a heavy partner of the Higgs boson, the particle discovered in 2012 at the Large Hadron Collider.

The higgsino is very heavy: about a thousand times heavier than a proton. But to bump into an atomic nucleus, it does not need high speed; it just needs to fly close by and give a slight push.

Scientists calculated what the interaction strength of the higgsino with a nucleus should be if its mass is around 1 TeV. The resulting number falls within the range measured by the detector. This means that the higgsino could leave exactly such a trace. But so far only one event has been recorded, and that is too few to confidently say: yes, this is dark matter. More data are needed to distinguish a fluke from a real signal.

The energy of the event, 248 keV, is about a million times smaller than the energy carried by protons in the Large Hadron Collider, yet such low-energy nuclear recoils could reveal the presence of heavy dark matter particles.

\sigma_{\tilde{H}N} = \frac{G_F^2 \mu_N^2}{8\pi} \simeq 1.86 \times 10^{-39} \text{ cm}^2
The higgsino-nucleon interaction cross section is determined by the Fermi constant and the reduced mass of the higgsino-nucleon system.
\delta \simeq m_Z^2 \left( \frac{\sin^2 \theta_W}{M_1} + \frac{\cos^2 \theta_W}{M_2} \right)
The mass splitting between the two neutral higgsino states depends on the Z boson mass, the bino and wino masses, and the Weinberg angle.
Scientists
Fritz ZwickyVera RubinRoberto D. PecceiHelen QuinnR. Brent Tully
Concepts
lz nuclear recoil sterile neutrino dark matter neutrino dark matter interactions liquid xenon borexino tau lepton lead nucleus supernova nucleosynthesis halo nuclei hidden particle decay z boson neutrinoless double beta decay xenonnt platinum axion kilonova high energy neutrino ultralight dark matter