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/*
* Main code for reading output files from stationary axisymmetric rotating stars.
*
*/
/*
* Copyright (c) 2010 Frederic Vincent
*
* This file is part of LORENE.
*
* LORENE is free software; you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation; either version 2 of the License, or
* (at your option) any later version.
*
* LORENE is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with LORENE; if not, write to the Free Software
* Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA
*
*/
char read_star_C[] = "$Header: /cvsroot/Lorene/Codes/Nrotstar/read_star.C,v 1.2 2014/10/13 08:53:58 j_novak Exp $" ;
/*
* $Id: read_star.C,v 1.2 2014/10/13 08:53:58 j_novak Exp $
* $Log: read_star.C,v $
* Revision 1.2 2014/10/13 08:53:58 j_novak
* Lorene classes and functions now belong to the namespace Lorene.
*
* Revision 1.1 2010/03/22 12:44:55 f_vincent
* Added read_star.C for reading output files computed by nrotstar.C
*
*
*
* $Header: /cvsroot/Lorene/Codes/Nrotstar/read_star.C,v 1.2 2014/10/13 08:53:58 j_novak Exp $
*/
// C headers
#include <cstdlib>
#include <cmath>
#include <cstring>
// Lorene headers
#include "star_rot.h"
#include "eos.h"
#include "utilitaires.h"
#include "graphique.h"
#include "nbr_spx.h"
#include "unites.h"
using namespace Lorene ;
int main(){
FILE* res=fopen("resu.d","r");
Mg3d mg(res);
cout << "mg= " << mg << endl;
Map_et mp(mg,res);
cout << "mp= " << mp << endl;
Eos* p_eos = Eos::eos_from_file(res);
cout << "eos=" << *p_eos << endl;
Star_rot star(mp,*p_eos,res);
star.equation_of_state();
star.update_metric();
star.hydro_euler();
cout << "star=" << star << endl;
Metric gg=star.get_gamma();
cout << "metric=" << gg << endl;
Scalar g_11=gg.cov()(1,1);
cout << "g11=" << g_11.val_point(1.,M_PI,0.) << endl;
Scalar d1g11=g_11.dsdr();
cout << "der " << d1g11.val_point(1.,M_PI,0.) << endl;
}
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