The free-streaming length of dark matter depends on fundamental dark matter physics, and
determines the abundance and concentration of dark matter haloes on sub-galactic scales …

Using a single gravitational lens system observed at≲ 5 mas resolution with very long
baseline interferometry, we place a lower bound on the mass of the fuzzy dark matter (FDM) …

We derive joint constraints on the warm dark matter (WDM) half-mode scale by combining
the analyses of a selection of astrophysical probes: strong gravitational lensing with …

Core formation and runaway core collapse in models with self-interacting dark matter (SIDM)
significantly alter the central density profiles of collapsed haloes. Using a forward modelling …

Strong lensing provides a powerful means of investigating the nature of dark matter as it
probes dark matter structure on sub-galactic scales. We present an extension of a forward …

We use a sample of 17 strong gravitational lens systems from the BELLS GALLERY survey
to quantify the amount of low-mass dark matter haloes within the lensing galaxies and along …

We investigate the mass structure of a strong gravitational lens galaxy at z= 0.350, taking
advantage of the milliarcsecond (mas) angular resolution of very long baseline …

Ultra-light dark matter (ULDM) refers to a class of theories, including ultra-light axions, in
which particles with mass comprise a significant fraction of the dark matter. A galactic scale …

Strong-gravitational lens systems with quadruply imaged quasars (quads) are unique
probes to address several fundamental problems in cosmology and astrophysics. Although …

We use the observed amount of subhaloes and line-of-sight dark matter haloes in a sample
of 11 gravitational lens systems from the Sloan Lens ACS Survey to constrain the free …