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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.

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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
 * NNDC Cluster
 * Calculation Logs
 * Nuclear Data Libraries
 * NuPYCEE
 * NuSE
 * Using GitHub
 * MESA
 * CANFAR
 * Discussion with Marco
 * 22Ne_an_Project
 * Binary Stars
 * SkyNet
 * Xnet
 * GALPROP
 * Useful links