Probing dark matter substructure with astrometric weak lensing

Abstract: Low-mass structures of dark matter are expected to be entirely devoid of light-emitting regions and baryons. Precisely because of this lack of baryonic feedback, small-scale substructures of the Milky Way are a relatively pristine testing ground for discovering aspects of dark matter microphysics and primordial fluctuations on sub-galactic scales. I will present results from the first search for galactic dark matter subhalos with time-domain astrometric weak gravitational lensing. The analysis is based on a matched-filter template of local lensing corrections to the proper motion of stars in the Magellanic Clouds and is most sensitive to compact dark structures of ten million to a hundred million solar mass.

HEP - phenomenologyHEP - theorymathematical physics

Audience: researchers in the topic

NHETC Seminar

Series comments: Description: Weekly research seminar of the NHETC at Rutgers University

Livestream link is available on the webpage.