The Small-Scale Structure of Galactic Dark Matter
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}} }
Massachusetts Institute of Technology (MIT) - Department of Physics
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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.