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====== r-process es su-process, s-process is our-process: ======

**Members:** Ali (analysis), Matt (code), Rob (parameters)

**Project:** Nuke Network:: "Simulate the s-process under AGB conditions. Compare to solar system abundances and presolar grains. How does the result depend on initial composition? How good is the waiting point approximation?"

[[http://dimit.me/Fe26/|Alternate network simulation.]]

[[http://i.imgur.com/xzAyngF.png|Overview]]\\

[[Inputs]] \\ [[https://docmgmt.nscl.msu.edu/share/page/site/TALENT/documentlibrary#filter=path%7CCourse7_2014/Projects/Project1/r-process%20es%20su-process%2C%20s-process%20is%20our-process/Data|Data (link to Document Server)]]\\
//The realout files contain mass fractions corresponding to atomic numbers beginning with Helium//\\ [[https://docmgmt.nscl.msu.edu/share/page/site/TALENT/documentlibrary#filter=path%7C/Course7_2014/Projects/Project1/r-process%2520es%2520su-process%252C%2520s-process%2520is%2520our-process/Results&page=1|Results (link to Document Server)]] \\ [[Code Revisions]] \\ [[Useful Links]]

Notes::

**May 30**\\
Big questions:\\
How do we simulate AGB environment in network code?\\
     -abundances of nuclei?
     -density, temp, pressure?
     -mass?\\
What are we going to include in the network?
     -take the entire chart of stable nuclides, and include "padding" on the neutron-rich side

**June 2**\\
Big questions:\\
     -Overall goals: explore how metallicity changes the progression of the s-process
     -Plan of attack:
         - edit sunet & run through the reducereaclib
         - run constant T calculation to validate appropriate network inputs and to debug
         - edit th_input to reflect AGB environment
     -Code additions/modifications:
         - th_input
         - sunet (all stable & some nuetron-rich)
         - eos selection (Bahcall is default - recompile for Helmholtz)
         - match.f90 (only relevant for MPI?)
         - matrix solver (backward Euler?)
     -Most useful visualizations:
         -abundances video?
         -comparison abundances to e.g. [[http://www.as.utexas.edu/~chris/halofield2.jpg|s-process abundance chart]].

**June 3**\\
-Successful implementation of the PARDISO sparse matrix solver into the Xnet code.\\
-[[Reaction network]] run through reaclib & reaction rates obtained.\\

**June 4**\\
-Test runs to check inputs\\
-Started creating presentation\\
-Created visualization of network\\
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