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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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</box> | </box> | ||
- | <box 80% left blue|**(During-Course Assignment)**> | ||
- | **Run a hydrodynamic code for:** | ||
- | |||
- | - 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#bnd|Bondi Accretion]] problem. | ||
- | - Gravitational collapse of: | ||
- | * Uniformly distributed “star” (P(initial) = 0) | ||
- | * Simple density profile (P(initial) = 0) | ||
- | * Are there self-similar solutions? | ||
- | - Energy injection into gas clump of: | ||
- | * uniformly distributed mass | ||
- | * simple density profile $\rho(r) = \rho(0)[1-(r/R)^2]^n $ | ||
- | * How does the evolution change with different injection energies | ||
- | - Drive a piston through some medium | ||
- | * Piston in a cylinder | ||
- | * Spherical piston driving outwards | ||
- | * Spherical piston driving inwards | ||
- | * How does the outward driven spherical piston compare to the energy injection? | ||
- | </box> | ||
~~DISCUSSION|Hydrodynamic Exercises Discussion~~ | ~~DISCUSSION|Hydrodynamic Exercises Discussion~~ |