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New Sensors Open Low Frequencies for Gravitational Waves ⚡ экспресс

Original: "Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz"
arXiv:2602.23531 · 2026-02-26 · CC BY 4.0 · ⏱ 1 min · Instrumentation
By suppressing the Earth's tremors, new sensors unlock low-frequency gravitational waves — a key to mid-sized black holes.
Abstract

The sensitivity of ground-based gravitational-wave detectors at frequencies below 20 Hz is limited by seismic noise and inertial sensor noise. Ultra-high-vacuum inertial isolation technologies and laser position sensors have been proposed, providing active platform stabilization down to 10 mHz. Laser sensor sensitivity reaches 10⁻¹² m/√Hz (polarization-independent), which is 100 times better than current LIGO sensors, and inertial sensors outperform commercial seismometers by at least a factor of 5. Simulations on a LIGO-type facility predict an improvement in low-frequency sensitivity of up to one order of magnitude at 10 Hz and a tripling of the detection horizon for binary systems of intermediate-mass black holes (10³ M☉). This is the first experimental confirmation of the feasibility of ground-based detectors operating below 10 Hz and the foundation for next-generation observatories (Cosmic Explorer, Einstein Telescope).

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Even Einstein predicted gravitational waves — a trembling of the very fabric of spacetime. Today they are captured by gigantic installations like LIGO, created thanks to Rainer Weiss and Kip Thorne. But all of them are a bit deaf to low notes: at frequencies below 20 oscillations per second, earthly shaking—from surf, trains, even walking people—drowns out the signal, like the noise of an orchestra muffling a quiet whisper.

New laser sensors are a hundred times more precise: they detect a displacement smaller than the size of an atomic nucleus.

The solution is a system that dampens the tremor, like active noise-canceling headphones, suppressing interference down to one-hundredth of an oscillation per second (10 millihertz). With motion sensors five times more accurate than usual, this gives a tenfold gain at a frequency of 10 hertz. Now we can hear the bass chords of the Universe—mergers of black holes of intermediate mass, thousands of times heavier than the Sun.

Future giants like Cosmic Explorer and Einstein Telescope are already being designed with this technology.

This dramatic leap will not only triple the search radius (volume — almost 30 times), but also possibly show whether supermassive black holes at the centers of galaxies grow from such "seeds".

🎯 Low-frequency gravitational waves are the only messenger from black holes with masses from hundreds to hundreds of thousands of suns; these "golden means" have hidden from all telescopes.

🎬 Like in 'Interstellar': the instruments sensed how space trembled from distant black holes. Now we hear that tremor with unimaginable clarity.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
gravitational waves black hole spacetime curvature
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsequivalence principleno-hair theorem
Original: arXiv:2602.23531 · CC BY 4.0 · bridge42worlds