Page 5: Research news on Gravitational lensing

Gravitational lensing as a research area investigates the deflection, magnification, and distortion of light from distant sources by intervening mass distributions, as predicted by general relativity, and develops methods to use these effects as astrophysical and cosmological probes. It encompasses strong, weak, and microlensing regimes, focusing on reconstructing mass profiles of galaxies and clusters, mapping dark matter, constraining dark energy via lensing statistics and cosmic shear, and testing gravity on large scales. The field integrates theoretical modeling, numerical simulations, and analysis of large imaging and spectroscopic surveys, emphasizing inverse problems, bias control, and statistical inference to extract cosmological parameters and substructure properties.

A dramatic Einstein ring seen by Webb

One of the first verified predictions of general relativity is the gravitational deflection of starlight. The effect was first observed in 1919 during a total solar eclipse. Since stars appear as points of light, the effect ...

Mapping cosmic shear to illuminate dark energy

Gravitational lensing often evokes images of a cosmic funhouse mirror: duplicated galaxies, dramatic arcs and distorted shapes. But the web-like, large-scale structure throughout the universe also bends light in a weaker, ...

Euclid discovers a stunning Einstein ring

Euclid blasted off on its six-year mission to explore the dark universe on 1 July 2023. Before the spacecraft could begin its survey, the team of scientists and engineers on Earth had to make sure everything was working properly.

page 5 from 6