| Research
projects in CCMA |
กก- Software
projects for the theory of partitions,
(George
Andrews)
- High order
numerical methods for hyperbolic conservation laws by vanishing
viscosity, (Alberto
Bressan, Wen Shen,
Jinchao Xu and Zhengfu Xu)
- Modeling and
simulations of multiscale problems in complex fluids and biology,
(Qiang
Du, Chun Liu and
Andrew Belmonte)
-
Scientific computation and visualization
play critical roles in much of our on-going research collaboration,
ranging from investigating the geometric deformation and topological
transformation of elastic cellular membranes, studying complex
viscoelastic fluids, to understanding of defects in liquid crystals and
quantized vortices in superconductors and Bose-Einstein condensate.
- Computation
with a nonlinear dynamic programming problem,
(Jenny
Li)
- Modeling
mechanical behavior of solids, (Xiantao
Li)
-
A multiscale method will be developed for
crystalline solids, including a domain decomposition technique that
divides the computational domain into continuum regions where nonlinear
elasticity is applied and atomistic regions where molecular statics/dynamics
is used to reflect microscale configuration. The atomistic and continuum
models are coupled through a transparent boundary condition at the
interface.
- Algebraic
multigrid for fully discrete physical models,
(Xiantao
Li, Alexei Novikov,
Jinchao Xu and
Ludmil Zikatanov)
- Improved
Subgrid-Scale Modeling of Turbulent flows,
(Alexei
Novikov)
-
Adaptive and
multigrid methods for simulations of fuel cells,
(Pengtao
Sun, Chao-Yang
Wang, Jinchao Xu and
Guangri Xue)
-
Advanced numerical techniques will be
developed for a set of fuel cell model partial differential equations
that feature anisotropy, degeneracy, discontinuity, nonlinearity and
coupling between different physical components.
- Dynamics of
Population Models, (H.
Weiss)
-
Black Hole Simulation,
(Carlos
F. Sopuerta, Pengtao Sun,
Pablo
Laguna and
Jinchao Xu)
-
Extreme mass ratio binary
systems, binaries involving stellar mass objects orbiting
massive black holes, are considered to be a primary source of
gravitational radiation to be detected by the space-based
interferometer LISA. The numerical modeling of these binary
systems is extremely challenging because the scales involved
expand over several orders of magnitude. One needs to handle
large wavelength scales comparable to the size of the massive
black hole and, at the same time, to resolve the scales in the
vicinity of the small companion where radiation reaction effects
play a crucial role. Adaptive finite element methods, in which
quantitative control of errors is achieved automatically by
finite element mesh adaptivity based on posteriori error
estimation, are a natural choice that has great potential for
achieving the high level of adaptivity required in these
simulations. To demonstrate this, we present the results of
simulations of a toy model, consisting of a point-like source
orbiting a black hole under the action of a scalar gravitational
field.
-
Two Phase Flows,
(Andrew Belmonte, Chun Liu,
Pengtao Sun and Jinchao Xu)
- The research on this project is supported in part by the National Science
Foundation: Award No. DMS-0074299, DMS-0209497, and SCREMS award
No. DMS-0215392
-
Mesh Adaptation, (Long
Chen, Pengtao Sun and Jinchao
Xu)
- The research on this project is supported in part by the National Science
Foundation: Award No. DMS-0074299, DMS-0209497, and SCREMS Award No. DMS-0215392
- Theory
and application of subspace correction methods,
(Jinchao
Xu, Ludmil Zikatanov
)
- The research on this project is supported by the National Science Foundation: Award No. DMS-0074299 and DMS-0209497
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