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 Application Catalog |
ZEUS-MP/2
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ZEUS-MP/2 is the latest addition to the ZEUS line of community application codes developed by the Laboratory for Computational Astrophysics. The "MP" suffix denotes the "multi-physics," "massively parallel," and "message passing" aspects of the code. Self-gravity is supported in all dimensions and can be calculated with a variety of methods, depending on geometry, dimensionality, and boundary conditions. Methods include: (1) GM/r on 1D or 2D spherical grids; (2) a conjugate-gradient Poisson solver on 2D or 3D spherical and cylindrical grids; (3) a multigrid-based Poisson solver on 3D cartesian grids with non-periodic boundary conditions, and (4) a Fast Fourier Transform solver for 3D cartesian grids with triply-periodic boundaries. External point-mass potentials are also supported.
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Category: Life Sciences
Sub Category: Computational Fluid Dynamics
Publisher: Laboratory for Computational Astrophysics, University of California, San Diego
Date Published: March 16, 2007
Version: 2.1.2
Pricing:
License: Free
Runtime:
$1/CPU-hr.
What is a CPU-hr.?
A CPU-hr. is the aggregate CPU time spent across all machines, rounded up to the nearest hour (e.g., a task running on 1,000 CPUs for one minute = 1,000 CPU minutes or approximately 17 CPU hours, costing you only $17).
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Key Features
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- The physics suite in this release of ZEUS-MP includes gas hydrodynamics, ideal MHD, flux-limited radiation diffusion, self gravity, and multispecies advection.
- Hydrodynamic, radiation-hydrodynamic (RHD), and magnetohydrodynamic (MHD) simulations can be performed on 1, 2, or 3-dimensional grids.
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Description |
ZEUS-MP/2 is the latest addition to the ZEUS line of community application codes developed by the Laboratory for Computational Astrophysics. The "MP" suffix denotes the "multi-physics," "massively parallel," and "message passing" aspects of the code. Self-gravity is supported in all dimensions and can be calculated with a variety of methods, depending on geometry, dimensionality, and boundary conditions. Methods include: (1) GM/r on 1D or 2D spherical grids; (2) a conjugate-gradient Poisson solver on 2D or 3D spherical and cylindrical grids; (3) a multigrid-based Poisson solver on 3D cartesian grids with non-periodic boundary conditions, and (4) a Fast Fourier Transform solver for 3D cartesian grids with triply-periodic boundaries. External point-mass potentials are also supported. |
Technical Information |
Developer Web Page |
Publisher Information |
Laboratory for Computational Astrophysics, University of California, San Diego |
Pricing and Payment Information |
License: Free
Order Information: N/A
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Support: |
Mailing List Support: N/A
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