APA

Vogelsberger, M. (2011). The Small-Scale Structure of Galactic Dark Matter. Perimeter Institute. https://pirsa.org/11090103

MLA

Vogelsberger, Mark. The Small-Scale Structure of Galactic Dark Matter. Perimeter Institute, Sep. 23, 2011, https://pirsa.org/11090103

BibTex

@misc{ pirsa_PIRSA:11090103,
  doi = {10.48660/11090103},
  url = {https://pirsa.org/11090103},
  author = {Vogelsberger, Mark},
  keywords = {Particle Physics},
  language = {en},
  title = {The Small-Scale Structure of Galactic Dark Matter},
  publisher = {Perimeter Institute},
  year = {2011},
  month = {sep},
  note = {PIRSA:11090103 see, \url{https://pirsa.org}}
}
            

Abstract

In my talk I will discuss the relevant astrophysical input for dark matter detection experiments, i.e. the expected distribution of dark matter at the solar position. Based on high resolution N-body simulations I will then show that the formation history of the galactic dark matter halo leaves imprints in the velocity and energy distribution. In the second part of my talk I will focus on the fine-grained dark matter structure and discuss the importance of caustics and streams for detection experiments.