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/*
* Main code for computation of binary black hole quasiequilibrium
* configurations
*
*
*/
/*
* Copyright (c) 2005 Philippe Grandclement
*
* 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 version 2
* as published by the Free Software Foundation.
*
* 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 coal_bh_mdiff_C[] = "$Header: /cvsroot/Lorene/Codes/Bin_BH_mass_diff/coal_bh_mdiff.C,v 1.3 2014/10/13 08:53:52 j_novak Exp $" ;
/*
* $Id: coal_bh_mdiff.C,v 1.3 2014/10/13 08:53:52 j_novak Exp $
* $Log: coal_bh_mdiff.C,v $
* Revision 1.3 2014/10/13 08:53:52 j_novak
* Lorene classes and functions now belong to the namespace Lorene.
*
* Revision 1.2 2014/10/06 15:09:41 j_novak
* Modified #include directives to use c++ syntax.
*
* Revision 1.1 2005/08/29 15:10:19 p_grandclement
* Addition of things needed :
* 1) For BBH with different masses
* 2) Provisory files for the mixted binaries (Bh and NS) : THIS IS NOT
* WORKING YET !!!
*
* $Header: /cvsroot/Lorene/Codes/Bin_BH_mass_diff/coal_bh_mdiff.C,v 1.3 2014/10/13 08:53:52 j_novak Exp $
*
*/
#include "headcpp.h"
//standard
#include <cstdlib>
#include <cmath>
// LORENE
#include "type_parite.h"
#include "nbr_spx.h"
#include "proto.h"
#include "coord.h"
#include "tenseur.h"
#include "bhole.h"
#include "utilitaires.h"
#include "graphique.h"
using namespace Lorene ;
int main(int argc, char** argv) {
// Lecture du fichier de parametres :
if (argc <3) {
cout <<" Passer nom des fichiers en arguments SVP !" << endl ;
abort() ;
}
char* name_fich = argv[2] ;
FILE* fich = fopen(name_fich, "r") ;
Mg3d grille_un (fich) ;
Mg3d grille_deux (fich) ;
Map_af map_un (grille_un, fich) ;
Map_af map_deux (grille_deux, fich) ;
Bhole hole_un (map_un, fich) ;
Bhole hole_deux (map_deux, fich) ;
fclose(fich) ;
char blabla [120] ;
name_fich = argv[1] ;
ifstream param(name_fich) ;
double precis, relax, search_ome, m1, m2 ;
int nbr_ome ;
param >> m1 ; param >> m2 ; param.getline(blabla, 120) ;
param >> search_ome ; param.getline(blabla, 120) ;
param >> precis ; param.getline(blabla, 120) ;
param >> relax ; param.getline(blabla, 120) ;
param >> nbr_ome ; param.getline(blabla, 120) ;
param.close() ;
// Le fichier sortie pour la recherche de omega :
Bhole_binaire bin (map_un, map_deux) ;
bin.set(1) = hole_un ;
bin.set(2) = hole_deux ;
bin.set_omega(0) ;
bin.set(1).fait_n_comp (bin(2)) ;
bin.set(1).fait_psi_comp (bin(2)) ;
bin.set(2).fait_n_comp (bin(1)) ;
bin.set(2).fait_psi_comp (bin(1)) ;
bin.fait_decouple() ;
bin.fait_tkij() ;
double distance = bin(1).get_mp().get_ori_x() - bin(2).get_mp().get_ori_x() ;
cout << "CALCUL AVEC L = " << distance << endl ;
bin.coal (precis, relax, nbr_ome, search_ome, m1, m2, 1) ;
char name[20] ;
sprintf(name, "bin.dat") ;
FILE* fich_sortie = fopen(name, "w") ;
grille_un.sauve(fich_sortie) ;
grille_deux.sauve(fich_sortie) ;
map_un.sauve(fich_sortie) ;
map_deux.sauve(fich_sortie) ;
bin(1).sauve(fich_sortie) ;
bin(2).sauve(fich_sortie) ;
fclose(fich_sortie) ;
return 0 ;
}
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