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author | rhaas <rhaas@8e189c6b-2ab8-4400-aa02-70a9cfce18b9> | 2014-03-13 03:02:11 +0000 |
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committer | rhaas <rhaas@8e189c6b-2ab8-4400-aa02-70a9cfce18b9> | 2014-03-13 03:02:11 +0000 |
commit | 83e3c939ad5c62a1c745cefa49daf6b04df54940 (patch) | |
tree | 0a027f3b508b668f3769aeb8538d6eb4528a915c | |
parent | ae4ca16a00a0f48fd60a7431edab6f3250cbde69 (diff) |
EOS_Omni: update documentationsvn
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEOS/EOS_Omni/trunk@106 8e189c6b-2ab8-4400-aa02-70a9cfce18b9
-rw-r--r-- | doc/documentation.tex | 19 |
1 files changed, 16 insertions, 3 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index 8bbee49..65d5e86 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -113,9 +113,10 @@ Erik Schnetter \textless eschnetter@perimeterinstitute.ca\textgreater} interface and implements multiple analytic EOS, and also provides table reader and interpolation routines for finite-temperature microphysical EOS available from - \url{http://www.stellarcollapse.org}. Currently, the implemented - analytic EOS are the polytropic EOS, the gamma-law EOS, and a hybrid EOS - consisting of a 2-piece piecewise-polytrope with an a thermal, + \url{http://www.stellarcollapse.org}. In addition cold and barotropic + tabulated EOS are provided for use in initial data thorns. Currently, the + implemented analytic EOS are the polytropic EOS, the gamma-law EOS, and a + hybrid EOS consisting of a 2-piece piecewise-polytrope with a thermal, gamma-law component. \end{abstract} @@ -173,6 +174,7 @@ Here, for stellar core collapse simulations. \item \texttt{eoskey = 4}: Finite-temperature microphysical EOS \item \texttt{eoskey = 5}: Cold tabulated EOS with Gamma-Law + \item \texttt{eoskey = 6}: Tabulated barotropic EOS \end{itemize} \item \texttt{havetemp} determines whether the EOS is to be called as a function of $(\rho,\epsilon,Y_e)$ (\texttt{havetemp = 0}), or as a @@ -211,9 +213,20 @@ wrong. This is also true for the Einstein Toolkit GR hydro code \begin{verbatim} eos_omni::poly_gamma +eos_omni::poly_gamma_initial eos_omni::poly_k \end{verbatim} +The only non-obvious parameter here is \texttt{poly\_gamma\_initial}. +In most simulations it should not be set. +In simulations that are run with a different adiabatic index than +what was used to set up the initial data, \texttt{poly\_gamma} should +be the evolution value, and \texttt{poly\_gamma\_initial} should be the +initial data value. \texttt{EOS\_Omni} then rescales \texttt{poly\_k} such +that the \emph{cgs} value of \texttt{poly\_k} is the same for initial data and +evolution. Since the units of \texttt{poly\_k} +($[K] = \frac{\rm N}{\rm m^2} \left(\frac{\rm m^3}{\rm kg}\right)^{\Gamma}$) +depend on \texttt{poly\_gamma} this is not fully trivial. Check \texttt{param.ccl} for parameters for the other EOS\@. |