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Welcome to the wiki
This wiki will provide all information on running the NuGrid codes for the work at Texas A&M.

N.B.!! If you don't edit this wiki for more than 60 days, the wiki is closed and you cannot edit. In that case, you should try to fix by unchecking "closed" as wiki explains (since you are a beraucrant).

Goals of the projects
1. Make accurate calculations on impact of 22Ne(a,n) new data on s-process abundances in Massive stars and AGB stars --> PRC 2. Clarify why 22Ne(a,n) must be the neutron source (by studying impacts of other reactions) --> APJ

For achieving these (especially second) goals,

* Conclude from comprehensive point of view including observation data, meteorites (so study well these data). * Try changing different reactions related to producing neutron (e.g., (18(a,n), etc) and study if currently used nuclear reactions are reasonable - which is expertise of nuclear physicist

Short-term goals
By NuGrid Collaboration 9/1/2019
 * Make sure calculations make sense --> Done.
 * Finish preliminary calculations of massive star's and AGB star's s-process abundance with different 22Ne(a,n) reaction rates (and discuss with Marco in the meeting). --> Done.
 * Start writing a draft paper of PRC (especially finish introduction part).

Calculations
Important data are stored in DropBox

List of page:
 * Computers
 * Mattermost
 * NuPPN
 * MPPNP
 * NuGridPy
 * WENDI
 * Calculation Logs
 * Nuclear Data Libraries
 * NuPYCEE
 * NuSE
 * Using GitHub
 * MESA
 * CANFAR
 * Discussion with Marco
 * 22Ne_an_Project
 * Binary Stars
 * SkyNet
 * Xnet
 * GALPROP
 * Useful links