update to reflect NSE table interface

massive_star/GNUmakefile

@@ -17,7 +17,7 @@ USE_CXX_REACTIONS = TRUE
 
 USE_FORT_MICROPHYSICS = FALSE
 
-MAX_ZONES := 32768
+MAX_ZONES := 65536
 
 DEFINES += -DNPTS_MODEL=$(MAX_ZONES)
 

massive_star/README.md

@@ -1,21 +1,23 @@
+# massive star initial model
+
 This is the initial model routine for the massive star problem.
 
-The file: 15m_500_sec.txt is a 15 solar mass MESA initial model, with
+The file: `15m_500_sec.txt` is a 15 solar mass MESA initial model, with
 an aprox21 composition.
 
 It can be converted into the subset of nuclei for aprox19 via
-convert_21_to_19.py
+`convert_21_to_19.py`
 
 This setup uses Ye as the primary composition variable from the initial
 model in regions that are in NSE.
 
 Note: you should ensure that the NSE conditions in the inputs file match
 those of your simulation, so the model will be properly in HSE.
 
-Also note that when running with 32768 zones, you need to do:
+Also note that when running with > 16384 zones, you need to do:
 
 ```
-ulimit -s 16384
+ulimit -s 32768
 ```
 
-Since the arrays are put on the stack.
+since the arrays are put on the stack.

massive_star/init_1d.H

@@ -83,12 +83,18 @@ set_aux(eos_t& eos_state) {
         Real dbeadt_pass;
         Real e_nu_pass;
 
-        nse_interp(eos_state.T, eos_state.rho, eos_state.aux[AuxZero::iye],
-                   abar_pass, bea_pass,
-                   dyedt_pass, dabardt_pass, dbeadt_pass, e_nu_pass,
-                   eos_state.xn);
+	nse_table_t nse_state;
+	nse_state.T = eos_state.T;
+	nse_state.rho = eos_state.rho;
+	nse_state.Ye = eos_state.aux[AuxZero::iye];
 
-        eos_state.aux[AuxZero::iabar] = abar_pass;
+        nse_interp(nse_state);
+
+	for (int n = 0; n < NumSpec; ++n) {
+	    eos_state.xn[n] = nse_state.X[n];
+	}
+
+        eos_state.aux[AuxZero::iabar] = nse_state.abar;
 
     } else {
         set_aux_comp_from_X(eos_state);