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Use the table below to navigate this beast:
CHIMERA: CCSN 1D/2D/3D - and ECSN
with the development of three-dimensional simulations we are
1) working on accelerating the
nuclear network solutions in two significant ways; 1) by
spreading the network calculations
to multiple cores using a shared-memory spreading the network
calculations to multiple cores using a shared memory
parallel programming interface
called OpenMP and 2) taking advantage of quasi parallel programming
interface called OpenMP, and 2) taking advantage of quasi-statistical
equilibrium conditions during silicon burning to reduce the size of the
system of equations In combination
these approaches will allow self consistent system of equations. In
combination, these approaches will allow self-consistent nuclear
abundance simulations beyond any to date.
Trunk: This is the primary production of the code.
Branch: The current branch is an OpenMP implementation
wrapped Chimera's nuclear network with an OpenMP routine. We are
currently testing runs to enhance the efficiency of our simulations.
movie files: Data3/Model_n
To obtain a copy of chimera use:
Anthony Mezzacappa, Raph Hix, Bronson Messor, Eric Lentz, Merek Austin Chertkow, Suzanne Parete-Koon, Eric Lingerfelt.