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| | | | | Show pages from United States Show all pages | |
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 |  | A TIPSY file viewer with MPI capabilities
- http://hubble.sourceforge.net
- [Open source - Linux] "Hubble in a bottle!" is visualization software for N-body simulations, which can be run in parallel using MPI for visualizing very large simulation results. Simulation output must be in TIPSY format. | |
| | Aarseth's N-body software
- http://www.ast.cam.ac.uk/~sverre/
- [open source - multiplatform] Direct N-body algorithms. | |
| | Barnes & Hut Treecode Algorithm
- http://www.ifa.hawaii.edu/~barnes/software.html
- [open source - multiplatform] A guide to a tree code algorithm implementation, used for astronomical N-body simulations. | |
| | CAPGADGET
- http://www.geocities.com/capgadget/
- [open source - multiplatform] Visualization package to capture and display Gadget N-body simulations. | |
| | CMBEASY -- CMB calculations with Graphical User Interface
- http://www.cmbeasy.org/
- CMBEASY is a C++ code with GUI for calculation of CMB power spectra and other density fluctuation evolution data for a given cosmology. | |
| | COSMOMC-- Monte Carlo evaluation of CMB parameters
- http://cosmologist.info/cosmomc/
- COSMOMC calculates a fast Markov Chain Monte-Carlo exploration of cosmological parameter space for an input set of constraints. | |
| | Cloudy & Associates
- http://www.nublado.org/
- Cloudy is an extensive, well-established, large-scale spectral synthesis code designed to simulate fully physical conditions within an astronomical plasma and then predict the emitted spectrum. The web page contains links to papers published with cloudy, the most recent version of the software itself, and a discussion board. | |
| | DUSTY -- Radiation transfer through dust
- http://www.pa.uky.edu/~moshe/dusty/
- DUSTY calculates the emerging spectrum of radiation from some source viewed after processing by a dusty region. The original radiation is scattered, absorbed and reemitted by the dust, and the emerging processed spectrum often provides the only available information about the embedded object. DUSTY can handle both planar and centrally-heated spherical density distributions. The number of independent input model parameters is minimized by fully implementing the scaling properties of the radiative transfer problem, and the spatial temperature profile is found from radiative equilibrium at every point in the dusty region. DUSTY has built in optical properties for the most common types of astronomical dust and comes with a library for many other grains. | |
| | EZ Stellar Evolution
- http://www.kitp.ucsb.edu/~paxton/EZ-intro.html
- EZ (Evolve ZAMS) Stellar Evolution tracks the evolution of new (Zero-Age Main Sequence) stars throughout the bulk of their lives (until an event which EZ does not model occurs, such as a Helium Flash or core crystallization). The code is clean and well documented. Links include a web interface to the code. | |
| | Enzo
- http://cosmos.ucsd.edu/enzo/
- Enzo is an adaptive mesh refinement (AMR), grid-based hybrid code (hydro + N-Body) which is designed to do simulations of cosmological structure formation. |
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