Previous | Session 171 | Next | Author Index | Block Schedule
G. C. Jordan, N. Hearn, B. Gallacher, T. Plewa (ASC FLASH CENTER, University of Chicago)
Calculating the nucleosynthetic yields from large-scale hydrodynamical simulations of astrophysical phenomena (such as Type Ia supernovae) involves the post-processing of tracer particles that track the individual fluid elements in the object. The number of tracer particles in the simulation can be on the order of hundreds of thousands; however, the question of the number of tracer particles needed to accurately predict output of the nucleosynthesis has not been addressed. We present statistics that answer the question of how many tracer particles are needed and offer guidelines for those running particle enabled simulations, specifically in the context of turbulent combustion in Type Ia supernova settings.
If you would like more information about this abstract, please follow the link to http://flash.uchicago.edu. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: firstname.lastname@example.org
Previous | Session 171 | Next
Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.