Measurements from quantum devices, particularly transmon qubits, open new avenues for detecting dark matter interactions. Transmons suppress external noise while maintaining high sensitivity to ultra-small energy depositions. Dark matter particles from the galactic halo, scattering off electrons, can transfer energy to a qubit, shortening its decoherence time. Recent experiments have recorded a steady residual contribution to the decoherence rate that cannot be explained by thermal fluctuations or known external sources. Based on this data, the most stringent laboratory limits to date have been set on dark matter–electron scattering in the keV energy range, along with competitive limits on dark photon absorption. The result demonstrates the potential of solid-state quantum detectors as a tool for directly testing light dark matter models.
Dark matter is an invisible substance, five times more abundant in the universe than ordinary matter. Its particles barely touch atoms, but occasionally they can nudge an electron—like a string brushed by the wind.
At ultra-low temperatures, qubits in quantum computers are like taut strings: the slightest disturbance snaps their pure 'sound'. A dark matter particle colliding with an electron in such a device causes a jitter, increasing entropy and breaking the signal. John Bardeen explained superconductivity—the key to their operation.
By listening to this jitter in dozens of experiments, scientists filtered out ordinary noise and found a contribution that doesn't fit known physics. Thus they set record constraints on the properties of dark matter particles and their scattering off electrons, going beyond the Standard Model.
🎯 The energy from a dark matter particle's impact is so tiny it could only lift a grain of sand by the thickness of a human hair—yet even this drop disrupts the quantum string.
🎬 Science fiction writers dreamed of detectors for ghost particles. Quantum strings turned fantasy into reality, letting us hear the silent cosmos.