Cosmic Mirages Test the Law of Gravity ✎ express

Original: "Cosmological constraints on viable $$f(R)$$ models using weak lensing"
arXiv:2601.04048v1 · 2026-01-07 · arXiv non-exclusive · independent analysis · 1 min
Distorted light from distant galaxies helped test gravity theories that could replace dark energy.

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Light from distant galaxies, passing through clusters of matter, gets distorted — much like the bottom of a pool breaks up into ripples of water. Astronomers measure these barely perceptible bends in shape and create a map of gravitational ‘ripples.’ This is weak lensing — a natural detector of invisible matter. However, the accelerated expansion of the cosmos is usually attributed to dark energy, but maybe it’s not there, and gravity itself on huge scales works a little differently. By testing theories where gravity gets a tiny correction, scientists overlaid them onto the distortion map. It turned out that the allowed deviations from Einstein’s law are within a few percent. To spot the difference, they had to average the shapes of millions of galaxies. If gravity were different, the night’s constellations would ‘ripple’ differently, and it would be visible. So lensing became a judge, separating permissible corrections from fantasies.

When a distant quasar, a lensing galaxy, and a telescope line up, an Einstein ring appears, a perfectly round circle of light.

Scientists
Fritz ZwickyVera RubinJacob BekensteinKarl SchwarzschildJoseph WeberAdam Riess
Concepts
lambda cdm weak lensing dark energy alternatives ecdm model cosmological parameters cosmological constant problem cold dark matter alternative gravity theories cosmic expansion uncertainty quantum cosmology cosmic distance measurement gravitational lensing modeling expansion of the universe cosmology expanding universe quantum gravity and symmetry constraint energy conditions fermi telescope gravitational microlensing