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--- group10 [2014/06/02 14:05]
siegl
+++ group10 [2014/06/12 13:22] (current)
siegl
@@ Line 19: / Line 19: @@
 Determine theoretical astrophysical conditions for AGB stars during the s-process.
-Create reaction network for both <sup>56<sub>Fe and solar abundance seeds.
+Create reaction network for both <sup>56</sup>Fe and solar abundance seeds.
 Create toolkit to read binary file into format appropriate for abundance graphing.
 Modify xnet code to allow the definition of a time-dependent neutron flux.
+**Accomplishments:**
+We found a set of astrophysical conditions for the s-process in AGB stars, a temperature of 0.28GK and baryon density of 2.6e+3 g/cm^3.
+We incorporated those conditions into xnet reaction network with an initial abundance of <sup>4</sup>He and <sup>13</sup>C in order to produce neutrons and a 1% abundance of <sup>56</sup>Fe.
+We also developed a python script to extract the abundances at a time step from the xnet binary files.
+We then generated final abundances for iron concentrations of .1%, 1%, and 10%.
 **References**
+{{:sprocesskaeppler.pdf|}}
+{{:sprocesslugaro.pdf|}}
+final abundance format :
+Z[first column], A[second column], Y[third column]
+Presentation:
+{{::today.odp|}}

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