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- | ====== TALENT ====== | + | ====== EXERCISES ====== |
- | ===== Training in Advanced Low Energy Nuclear Theory: EXERCISES ===== | + | **[[RXNnetworkEX|Reaction Networks]]**, **[[NuclPhysInput|Nucl Physics Input]]**, **[[HydroEX|Hydro]]**, **[[BBNEX|BBN]]**, **[[AnlyPlot|Abundances, Analysis and Plotting]]** |
- | [[http://www.nucleartalent.org|{{:talent.png?650|Nuclear TALENT}}]] | + | |
- | **[[RXNnetworkEX|Reaction Networks]]**, **[[NuclPhysInput|Nucl Physics Input]]**, **[[HydroEX|Hydrodynamics]]**, **[[BBNEX|BBN]]**, **[[AnlyPlot|Abundances, Analysis and Plotting]]** | + | |
==== Abundances, Analysis and Plotting ==== | ==== Abundances, Analysis and Plotting ==== | ||
<box left 80% orange|**(Pre-Course Assignment)**> | <box left 80% orange|**(Pre-Course Assignment)**> | ||
- | **Analyze and plot abundances:** | + | **Analyze and plot Solar Abundances:** |
- Grab the solar system abundances and plot them | - Grab the solar system abundances and plot them | ||
+ | * Cite the data source (Anders & Grevesse, Lodders, Asplund, etc) | ||
* Vs mass number (A) | * Vs mass number (A) | ||
* Vs atomic number (Z) | * Vs atomic number (Z) | ||
- | - Grab stellar abundances from the [[http://saga.sci.hokudai.ac.jp/wiki/doku.php|SAGA Database]] for a handful of stars | + | |
- | * Plot abundances in [A/H] notation | + | **Analyze and plot Stellar Abundances** |
- | * Translate [A/H] notation into mass fraction abundances | + | - Grab stellar abundances from the [[http://saga.sci.hokudai.ac.jp/wiki/doku.php|SAGA Database]] for a handful of stars |
+ | $\ \ \ \ \ \ [A/B]= \log_{10}(A/B)_{star} - \log_{10}(A/B)_\odot$ | ||
+ | * Plot | ||
+ | - [Ca/H], [Ge/H], [Zr/H], [Sr/H], [Ba/H], [La/H], [Nd/H], [Eu/H] vs [Fe/H] | ||
+ | * Are these elements correlated with metallicity? | ||
+ | * Do they have the same correlation? | ||
+ | - [Ca/Fe], [Ge/Fe], [Zr/Fe], [Sr/Fe], [Ba/Fe], [La/Fe], [Nd/Fe] vs [Eu/Fe] | ||
+ | * Are these elements correlated with Eu? | ||
</box> | </box> |