Statistics – Computation
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20311113p&link_type=abstract
American Astronomical Society Meeting 203, #111.13; Bulletin of the American Astronomical Society, Vol. 36, p.582
Statistics
Computation
Scientific paper
Hydrodynamic instabilities play an important role in determining the morphology and evolution of astronomical entities. Any interface of discontinuous density is subject to instabilities, including Rayleigh-Taylor, Kelvin-Helmholtz, and a recently discovered instability driven by self-gravity. In an ongoing computational study, we seek to validate the linear theory developed for the self-gravity driven interfacial instability (SGI) and examine its nonlinear behavior. Here, we present the results from hydrodynamic simulations designed to expand the parameter space and investigate the effects of compressibility, perturbation strength, and Atwood number. We also look forward toward modeling coupled effects due to multiple instabilities.
Hueckstaedt Robert M.
Hunter James H. Jr.
Peterson A. H.
No associations
LandOfFree
Parameter space studies for the self-gravity interfacial instability does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Parameter space studies for the self-gravity interfacial instability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Parameter space studies for the self-gravity interfacial instability will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1422429