star_bin_global.C

/*
 * Methods for computing global quantities within the class Star_bin
 *
 * (see file star.h for documentation)
 */

/*
 *   Copyright (c) 2004 Francois Limousin
 *
 *   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 star_bin_global_C[] = "$Header: /cvsroot/Lorene/C++/Source/Star/star_bin_global.C,v 1.5 2005/09/13 19:38:31 f_limousin Exp $" ;

/*
 * $Id: star_bin_global.C,v 1.5 2005/09/13 19:38:31 f_limousin Exp $
 * $Log: star_bin_global.C,v $
 * Revision 1.5  2005/09/13 19:38:31  f_limousin
 * Reintroduction of the resolution of the equations in cartesian coordinates.
 *
 * Revision 1.4  2005/02/17 17:33:25  f_limousin
 * Change the name of some quantities to be consistent with other classes
 * (for instance nnn is changed to nn, shift to beta, beta to lnq...)
 *
 * Revision 1.3  2004/02/27 09:54:24  f_limousin
 * Generalisation of the formulas for mass_b and mass_g for non
 * conformally flat metrics.
 *
 * Revision 1.2  2004/01/20 15:18:17  f_limousin
 * First version
 *
 *
 * $Header: /cvsroot/Lorene/C++/Source/Star/star_bin_global.C,v 1.5 2005/09/13 19:38:31 f_limousin Exp $
 *
 */

// Headers C

// Headers Lorene
#include "star.h"
#include "utilitaires.h"

            //--------------------------//
            //  Baryon mass     //
            //--------------------------//

double Star_bin::mass_b() const {

    if (p_mass_b == 0x0) {    // a new computation is required

    Scalar det_gamma = gamma.determinant() ;
    
    Scalar dens = sqrt(det_gamma) * gam_euler * nbar ;

//  Scalar dens = psi4 * sqrt(psi4) * gam_euler * nbar ;
    
    dens.std_spectral_base() ; 
    
    p_mass_b = new double( dens.integrale() ) ;
    
    }
    
    return *p_mass_b ; 

} 



            //----------------------------//
            //  Gravitational mass    //
            //----------------------------//

double Star_bin::mass_g() const {

    if (p_mass_g == 0x0) {    // a new computation is required
    
    Scalar det_gamma = gamma.determinant() ;

    Scalar dens = sqrt(det_gamma) * nn
        * ( ener_euler + s_euler ) ;
    
    dens.std_spectral_base() ; 
    
    p_mass_g = new double( dens.integrale() ) ;

    }
    
    return *p_mass_g ; 

} 

        
            //----------------------------------//
            //  X coordinate of the barycenter  //
            //----------------------------------//


double Star_bin::xa_barycenter() const {

    if (p_xa_barycenter == 0x0) {    // a new computation is required
    
    Scalar xxa(mp) ; 
    xxa = mp.xa ;   // Absolute X coordinate
    xxa.std_spectral_base() ;

    Scalar det_gamma = gamma.determinant() ;

    Scalar dens = sqrt(det_gamma) * gam_euler * nbar * xxa ; 
    
    int nzone = mp.get_mg()->get_nzone() ;
    dens.annule_domain(nzone - 1) ;

    dens.std_spectral_base() ; 

    p_xa_barycenter = new double( dens.integrale() / mass_b() ) ;
    
    }
    
    return *p_xa_barycenter ; 

}

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