The Aquarius Project: Cold Dark Matter under a Numerical Microscope
APA
Navarro, J. (2009). The Aquarius Project: Cold Dark Matter under a Numerical Microscope. Perimeter Institute. https://pirsa.org/09020044
MLA
Navarro, Julio. The Aquarius Project: Cold Dark Matter under a Numerical Microscope. Perimeter Institute, Feb. 27, 2009, https://pirsa.org/09020044
BibTex
@misc{ pirsa_PIRSA:09020044, doi = {10.48660/09020044}, url = {https://pirsa.org/09020044}, author = {Navarro, Julio}, keywords = {Cosmology}, language = {en}, title = {The Aquarius Project: Cold Dark Matter under a Numerical Microscope}, publisher = {Perimeter Institute}, year = {2009}, month = {feb}, note = {PIRSA:09020044 see, \url{https://pirsa.org}} }
University of Victoria
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Abstract
I will report results from simulations of galaxy-scale dark halos of unprecedented numerical resolution. Convergence tests demonstrate detailed convergence for (sub)structures for over six decades in mass, enabling detailed forecasts of the expected dark matter signal both in Earth-bound direct-detection experiments as well as in indirect detection experiments which attempt to image dark matter annihilation radiation in gamma rays.