Cosmic Wake Exposes Hidden Motions express

Original: "First detection of the moving lens effect with ACT and DESI LS"
arXiv:2605.18938 · 2026-05-18 · CC BY 4.0 · 1 min
A subtle distortion in the afterglow of the Big Bang lets us map the full motion of galaxies, including their sideways drift.

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Moving clumps of galaxies and invisible dark matter create wakes in the afterglow of the Big Bang, like boats stirring a pond. This wake, the moving lens effect, is so subtle it shifts the light’s temperature by only a few millionths of a degree: comparable to detecting a candle’s heat from across a continent.

Now, combining two telescope surveys, astronomers have detected this sideways motion for the first time. Until now, we could only see how matter moves toward or away from us.

The signal is so clear that the chance it's random noise is less than one in a million.

Pair this with the Sunyaev-Zel'dovich effect, which tracks gas motion, and a full 3D velocity map emerges. Such maps will test the standard model of cosmic expansion and trace the hidden currents shaping our universe.

Original abstract

as written by the authors arXiv:2605.18938

The moving lens effect is a secondary CMB anisotropy induced by the transverse motion of gravitational potentials. We develop a Fourier-space cross-spectrum estimator that retains the scale dependence of the signal, and apply it to the Atacama Cosmology Telescope (ACT) DR6 CMB temperature maps and luminous red galaxies from the DESI Legacy Imaging Surveys. Using the foreground-reduced ACT NILC map, we find strong evidence for a non-zero amplitude of the cross-correlation $$b_{\rm ML} = 1.24 \pm 0.26$$ ($$4.8\sigma$$) for the extended sample and $$0.93 \pm 0.25$$ ($$3.7\sigma$$) for the main sample, both consistent with the halo-model prediction for the moving lens signal. Our Fourier-based pipeline enforces separation of scales between the reconstructed velocities and the cross-correlation, which we show is essential for foreground mitigation. The residual foreground contamination is expected to be significantly smaller than the signal from both simulations and the multi-frequency analysis presented in this paper. No curl-mode test exceeds $$2\sigma$$, and the results are robust across analysis variants. They constitute the first detection of the moving lens effect and unlock access to transverse velocities, a new cosmological probe. When combined with the kinematic Sunyaev-Zel'dovich effect, this provides a path toward mapping the three-dimensional velocity field of the Universe, opening a new avenue for probing the growth of structure and gravity on large scales.

The effect shifts the temperature of the oldest light by only a few millionths of a degree — like detecting a candle’s warmth from across a continent.

Mapping cosmic flows in 3D feels like stepping into the navigator's seat in 'Dune', where space travel depends on reading invisible currents.

Scientists
Rashid Alievich SunyaevFritz ZwickyRainer SachsAlbert A. MichelsonVera RubinHenri Poincaré
Concepts
act Lense–Thirring effect magneto optical kerr effect frame dragging light deflection apparent diffusion coefficient cosmic microwave background measurement microlensing kerr effect