Building of the C API GridFire can now be used from fotran using the gridfire_mod fortran module. This exposes the same, limited, set of funcitonality that the C API does.
80 lines
2.1 KiB
C
80 lines
2.1 KiB
C
#include "gridfire/extern/gridfire_extern.h"
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#include <stdio.h>
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#define NUM_SPECIES 8
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// Define a macro to check return codes
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#define CHECK_RET_CODE(ret, ctx, msg) \
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if (ret != 0 && ret != 1) { \
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printf("Error %s: %s\n", msg, gf_get_last_error_message(ctx)); \
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gf_free(ctx); \
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return 1; \
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}
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int main() {
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void* ctx = gf_init();
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const char* species_names[NUM_SPECIES];
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species_names[0] = "H-1";
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species_names[1] = "He-3";
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species_names[2] = "He-4";
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species_names[3] = "C-12";
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species_names[4] = "N-14";
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species_names[5] = "O-16";
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species_names[6] = "Ne-20";
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species_names[7] = "Mg-24";
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const double abundances[NUM_SPECIES] = {
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0.702616602672027,
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9.74791583949078e-06,
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0.06895512307276903,
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0.00025,
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7.855418029399437e-05,
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0.0006014411598306529,
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8.103062886768109e-05,
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2.151340851063217e-05
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};
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int ret = gf_register_species(ctx, NUM_SPECIES, species_names);
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CHECK_RET_CODE(ret, ctx, "SPECIES");
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ret = gf_construct_engine_from_policy(ctx, "MAIN_SEQUENCE_POLICY", abundances, NUM_SPECIES);
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CHECK_RET_CODE(ret, ctx, "MAIN_SEQUENCE_POLICY");
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ret = gf_construct_solver_from_engine(ctx, "CVODE");
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CHECK_RET_CODE(ret, ctx, "CVODE");
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double Y_out[NUM_SPECIES];
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double energy_out;
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double dEps_dT;
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double dEps_dRho;
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double mass_lost;
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ret = gf_evolve(
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ctx,
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abundances,
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NUM_SPECIES,
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1.5e7, // Temperature in K
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1.5e2, // Density in g/cm^3
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3e17, // Time step in seconds
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1e-12, // Initial time step in seconds
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Y_out,
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&energy_out,
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&dEps_dT,
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&dEps_dRho, &mass_lost
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);
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CHECK_RET_CODE(ret, ctx, "EVOLUTION");
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printf("Evolved abundances:\n");
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for (size_t i = 0; i < NUM_SPECIES; i++) {
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printf("Species %s: %e\n", species_names[i], Y_out[i]);
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}
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printf("Energy output: %e\n", energy_out);
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printf("dEps/dT: %e\n", dEps_dT);
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printf("dEps/dRho: %e\n", dEps_dRho);
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printf("Mass lost: %e\n", mass_lost);
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gf_free(ctx);
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return 0;
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} |