How much dark matter really matters?
摘要
Strong gravitational lensing is a key probe to trace dark matter. It assumes that mass curves spacetime so that light from a background source is deflected on its way to the observer. If dark matter contributes the major part to a massive cosmic structure, reconstructing the latter from strong-lensing observables allows us to infer characteristics of dark matter. Standard reconstructions fit a pre-defined mass-density model to the data. In this essay, I show how these mass models over-estimate the dark-matter contents of light-deflecting masses. Eliminating these models from the reconstruction reveals that observations directly constrain local properties of light-deflecting masses. How much dark matter is really needed in strong-gravitational-lensing effects and how much do we make up by our model choices?
引用
@article{arxiv.2605.12593,
title = {How much dark matter really matters?},
author = {Jenny Wagner},
journal= {arXiv preprint arXiv:2605.12593},
year = {2026}
}
备注
Honorable mention in the Gravity Research Foundation Essay Contest