======Group 10======

**Topic**

Simulation of the s-process under AGB conditions in a nuclear reaction network

**Members**

Julia Bliss - Analysis

Jianping Lai - Parameters

Kevin Siegl - Code

====Log====

**Initial Goals:**

Determine theoretical astrophysical conditions for AGB stars during the s-process.

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|}}