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hydroex [2014/05/02 13:24] cyburt |
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===== Training in Advanced Low Energy Nuclear Theory: EXERCISES ===== | ===== Training in Advanced Low Energy Nuclear Theory: EXERCISES ===== | ||
[[http://www.nucleartalent.org|{{:talent.png?650|Nuclear TALENT}}]] | [[http://www.nucleartalent.org|{{:talent.png?650|Nuclear TALENT}}]] | ||
- | [[RXNnetworkEX|Reaction Networks]], [[HydroEX|Hydrodynamics]], [[BBNEX|BBN]], [[AnlyPlot|Abundances, Analysis and Plotting]], [[NuclPhysInput|Nuclear Physics Input]] | + | **[[RXNnetworkEX|Reaction Networks]]**, **[[HydroEX|Hydrodynamics]]**, **[[BBNEX|BBN]]**, **[[AnlyPlot|Abundances, Analysis and Plotting]]**, **[[NuclPhysInput|Nucl Physics Input]]** |
==== Hydrodynamic Exercises ==== | ==== Hydrodynamic Exercises ==== | ||
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**Download, compile and run the Hydrodynamics Code** | **Download, compile and run the Hydrodynamics Code** | ||
- | - Download the [[hydrocode|Hydrodynamics Code]]. | + | - Download the VH1.0 [[hydrocode|Hydrodynamics Code]]. |
- Compile the code with your fortran90 compiler. | - Compile the code with your fortran90 compiler. | ||
- Report in the Hydrodynamics Code discussion thread your success with machine information. | - Report in the Hydrodynamics Code discussion thread your success with machine information. | ||
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- Read the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php|Problems & Solutions]] guide. | - Read the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php|Problems & Solutions]] guide. | ||
- | * Set up and run the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php#stb|Sedov Blast]] problem. | + | - Set up and run the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php#stb|Sedov Blast]] problem. |
- | * Set up and run the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php#bnd|Bondi Accretion]] problem. | + | - Set up and run the [[http://astro.physics.ncsu.edu/pub/VH-1/bproblems.php#bnd|Bondi Accretion]] problem. |
- Gravitational collapse of: | - Gravitational collapse of: | ||
* Uniformly distributed “star” (P(initial) = 0) | * Uniformly distributed “star” (P(initial) = 0) |