PoS - Proceedings of Science
Volume 337 - Neutrino Oscillation Workshop (NOW2018) - Session V: Particle Physics in the Cosmos
Learning about Dark Matter from the Stars
J. Kopp
Full text: pdf
Published on: April 24, 2019
We discuss several novel astrophysical methods for elucidating the nature and the distribution of dark matter in the Universe. First, we argue that subhalos of the Milky Way's dark matter halo traveling through the disk will leave a characteristic imprint in the motion of nearby stars. These "stellar wakes" can be probed using precise astrometric data, for instance from Gaia. In the second part of the talk, we illustrate how gravitational lensing and pulsar timing can constrain compact dark matter objects such as primordial black holes or axion mini-clusters. Finally, we comment on the prospects of probing the dark sector using gravitational wave signals form neutron star mergers.
DOI: https://doi.org/10.22323/1.337.0081
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.