Jeff Kanipe
Abstract
With the help of supercomputers, scientists are now able to create models of large-scale astronomical events.
- Guedes, J., Callegari, S., Madau, P., and Mayer, L. Forming realistic late-type spirals in a ¿CDM universe: The Eris simulation, The Astrophysical Journal 742, 2, Dec. 2011.Google Scholar
Cross Ref
- Nordhaus, J., Brandt, T. D., Burrows, A., Almgren, A. The hydrodynamic origin of neutron kick stars, http://arxiv.org/abs/1112.3342.Google Scholar
- Prada, F., Klypin, A., Cuesta, A., Betancort-Rijo, J., and Primack, J. Halo concentrations in the standard ¿CDM cosmology, http://arxiv.org/pdf/1104.5130.pdf.Google Scholar
- Rantsiou, E., Burrows, A., Nordhaus, J., and Almgren, A. Induced rotation in 3D simulations of Ccre collapse supernovae: Implications for pulsar spins, The Astrophysical Journal 732, 1, May 2011.Google ScholarCross Ref
- University of California High-Performance AstroComputing Center Bolshoi videos, http://hipacc.ucsc.edu/ Bolshoi/Movies.html.Google Scholar
Index Terms
- Cosmic simulations
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