star.C

/*
 * Methods of class Star
 *
 * (see file star.h for documentation)
 */
 
/*
 *   Copyright (c) 2004 Francois Limousin
 *  
 *   Copyright (c) 2000-2001 Eric Gourgoulhon (for preceding class Etoile)
 *   Copyright (c) 2000-2001 Keisuke Taniguchi (for preceding class Etoile)
 *
 *   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
 *
 */
 
 
 
 
/*
 * $Id: star.C,v 1.22 2016/12/05 16:18:14 j_novak Exp $
 * $Log: star.C,v $
 * Revision 1.22  2016/12/05 16:18:14  j_novak
 * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
 *
 * Revision 1.21  2014/10/13 08:53:37  j_novak
 * Lorene classes and functions now belong to the namespace Lorene.
 *
 * Revision 1.20  2013/04/20 20:56:15  m_bejger
 * Fix for three domains in star in Star::equation_of_state from Etoile/etoile.C
 *
 * Revision 1.19  2010/02/02 12:45:16  e_gourgoulhon
 * Improved the display (operator>>)
 *
 * Revision 1.18  2010/01/26 16:49:03  e_gourgoulhon
 * Commented the test on the relativistic character of the EOS: the
 * relativity parameter is not defined (yet !) in the base class Star.
 *
 * Revision 1.17  2007/11/06 16:22:03  j_novak
 * The data member stress_euler is now a Sym_tensor instead of a Tensor.
 *
 * Revision 1.16  2007/06/21 19:53:47  k_taniguchi
 * Addition of p_ray_eq_3pis2
 *
 * Revision 1.15  2005/09/14 12:30:52  f_limousin
 * Saving of fields lnq and logn in class Star.
 *
 * Revision 1.14  2005/09/13 19:38:31  f_limousin
 * Reintroduction of the resolution of the equations in cartesian coordinates.
 *
 * Revision 1.13  2005/02/17 17:29:04  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 1.12  2005/01/05 17:43:03  f_limousin
 * u_euler is now constructed in the spherical triad to be consistent
 * with all the others vectors ans tensors.
 *
 * Revision 1.11  2004/11/11 16:29:49  j_novak
 * set_der_0x0 is no longer virtual (to be coherent with Tensor/Scalar classes).
 *
 * Revision 1.10  2004/06/22 12:48:08  f_limousin
 * Change qq, qq_auto and qq_comp to beta, beta_auto and beta_comp.
 *
 * Revision 1.9  2004/06/07 16:21:35  f_limousin
 * Add outputs
 *
 * Revision 1.8  2004/04/08 16:32:10  f_limousin
 * The new variable is ln(Q) instead of Q=psi^2*N. It improves the
 * convergence of the code.
 *
 * Revision 1.7  2004/03/25 10:29:26  j_novak
 * All LORENE's units are now defined in the namespace Unites (in file unites.h).
 *
 * Revision 1.6  2004/03/08 11:48:00  f_limousin
 * Error in del_deriv() and set_der_0x0() : p_mass_b and p_mass_g were
 * missing. And so they were never recomputed.
 *
 * Revision 1.5  2004/02/27 09:36:46  f_limousin
 * u_euler is now constructed on a cartesian basis instead
 * of a spherical one.
 *
 * Revision 1.4  2004/02/21 17:05:13  e_gourgoulhon
 * Method Scalar::point renamed Scalar::val_grid_point.
 * Method Scalar::set_point renamed Scalar::set_grid_point.
 *
 * Revision 1.3  2004/01/20 15:16:58  f_limousin
 * First version
 *
 *
 * $Header: /cvsroot/Lorene/C++/Source/Star/star.C,v 1.22 2016/12/05 16:18:14 j_novak Exp $
 *
 */
 
// Headers C
#include "math.h"
 
// Headers Lorene
#include "star.h"
#include "eos.h"
#include "utilitaires.h"
#include "param.h"
#include "unites.h"
 
 
                //--------------//
                // Constructors //
                //--------------//
 
// Standard constructor
// --------------------
namespace Lorene {
Star::Star(Map& mpi, int nzet_i, const Eos& eos_i)
         : mp(mpi), 
           nzet(nzet_i), 
           eos(eos_i), 
           ent(mpi), 
           nbar(mpi), 
           ener(mpi), 
           press(mpi),  
           ener_euler(mpi), 
           s_euler(mpi), 
           gam_euler(mpi), 
           u_euler(mpi, CON, mp.get_bvect_spher()), 
           stress_euler(mpi, CON, mp.get_bvect_spher()),
           logn(mpi), 
           nn(mpi), 
           beta(mpi, CON, mp.get_bvect_spher()),
           lnq(mpi),
           gamma(mp.flat_met_spher()){
    
 
    // Check of the EOS
//     const Eos_poly_newt* p_eos_poly_newt = 
//              dynamic_cast<const Eos_poly_newt*>( &eos ) ; 
//    
//     const Eos_incomp_newt* p_eos_incomp_newt = 
//              dynamic_cast<const Eos_incomp_newt*>( &eos ) ; 
//    
// 
//     
//     if (p_eos_poly_newt != 0x0) {
//  cout << 
//      "Star::Star : the EOS Eos_poly_newt must not be employed"
//       << " for a relativistic star ! " << endl ; 
//  cout << "(Use Eos_poly instead)" << endl ; 
//  abort() ; 
//  }
//     if (p_eos_incomp_newt != 0x0) {
//  cout << 
//      "Star::Star : the EOS Eos_incomp_newt must not be employed"
//       << " for a relativistic star ! " << endl ; 
//  cout << "(Use Eos_incomp instead)" << endl ; 
//  abort() ; 
//     }
//  
    // Pointers of derived quantities initialized to zero : 
    set_der_0x0() ;
 
    // All the matter quantities are initialized to zero :
    nbar = 0 ; 
    ener = 0 ; 
    press = 0 ; 
    ent = 0 ; 
    ener_euler = 0 ; 
    s_euler = 0 ; 
    gam_euler = 1. ; 
    gam_euler.std_spectral_base() ; 
    u_euler.set_etat_zero() ; 
    stress_euler.set_etat_zero() ;
 
    // The metric is initialized to the flat one : 
    Metric flat(mp.flat_met_spher()) ;
    flat.cov() ;
    gamma = flat ;
 
    logn = 0 ; 
    nn = 1. ; 
    nn.std_spectral_base() ; 
    beta.set_etat_zero() ; 
    lnq = 0 ;
 
}
 
// Copy constructor
// ----------------
Star::Star(const Star& et) 
         : mp(et.mp), 
           nzet(et.nzet), 
           eos(et.eos), 
           ent(et.ent), 
           nbar(et.nbar), 
           ener(et.ener), 
           press(et.press),  
           ener_euler(et.ener_euler), 
           s_euler(et.s_euler), 
           gam_euler(et.gam_euler), 
           u_euler(et.u_euler), 
           stress_euler(et.stress_euler),
           logn(et.logn), 
           nn(et.nn), 
           beta(et.beta),
           lnq(et.lnq),
           gamma(et.gamma){
           
    set_der_0x0() ;
 
}
 
// Constructor from a file
// -----------------------
Star::Star(Map& mpi, const Eos& eos_i, FILE* fich)
         : mp(mpi), 
           eos(eos_i), 
           ent(mpi), 
           nbar(mpi), 
           ener(mpi), 
           press(mpi),  
           ener_euler(mpi), 
           s_euler(mpi), 
           gam_euler(mpi), 
           u_euler(mpi, CON, mp.get_bvect_spher()), 
           stress_euler(mpi, CON, mp.get_bvect_spher()), 
           logn(mpi, *(mpi.get_mg()), fich), 
           nn(mpi), 
           beta(mpi, CON, mp.get_bvect_spher()),
           lnq(mpi, *(mpi.get_mg()), fich),
           gamma(mpi.flat_met_spher()){
 
    // Star parameters
    // -----------------
 
    // nzet is read in the file:     
    int xx ; 
    fread_be(&xx, sizeof(int), 1, fich) ;   
    nzet = xx ;
            
    // Equation of state
    // -----------------
    
    // Read of the saved EOS
    Eos* p_eos_file = Eos::eos_from_file(fich) ; 
    
    // Comparison with the assigned EOS:
    if (eos != *p_eos_file) {
    cout << 
    "Star::Star(const Map&, const Eos&, FILE*) : the EOS given in "
    << endl << 
    " argument and that read in the file are different !" << endl ; 
    abort() ;  
    }
    
    // p_eos_file is no longer required (it was used only for checking the
    //  EOS compatibility)
    delete p_eos_file ;
    
    // Read of the saved fields:
    // ------------------------
    Scalar ent_file(mp, *(mp.get_mg()), fich) ; 
    ent = ent_file ; 
    u_euler.set_etat_zero() ; 
    stress_euler.set_etat_zero() ;
    nn = 1 ;
    beta.set_etat_zero() ;
 
    // Pointers of derived quantities initialized to zero 
    // --------------------------------------------------
    set_der_0x0() ;
    
}
 
                //------------//
                // Destructor //
                //------------//
 
Star::~Star(){
 
    del_deriv() ; 
 
}
 
 
            //----------------------------------//
            // Management of derived quantities //
            //----------------------------------//
 
void Star::del_deriv() const {
 
    if (p_mass_b != 0x0) delete p_mass_b ; 
    if (p_mass_g != 0x0) delete p_mass_g ; 
    if (p_ray_eq != 0x0) delete p_ray_eq ; 
    if (p_ray_eq_pis2 != 0x0) delete p_ray_eq_pis2 ; 
    if (p_ray_eq_pi != 0x0) delete p_ray_eq_pi ; 
    if (p_ray_eq_3pis2 != 0x0) delete p_ray_eq_3pis2 ;
    if (p_ray_pole != 0x0) delete p_ray_pole ; 
    if (p_l_surf != 0x0) delete p_l_surf ; 
    if (p_xi_surf != 0x0) delete p_xi_surf ; 
 
    Star::set_der_0x0() ; 
}               
 
 
 
 
void Star::set_der_0x0() const {
 
    p_mass_b = 0x0 ; 
    p_mass_g = 0x0 ; 
    p_ray_eq = 0x0 ; 
    p_ray_eq_pis2 = 0x0 ; 
    p_ray_eq_pi = 0x0 ; 
    p_ray_eq_3pis2 = 0x0 ;
    p_ray_pole = 0x0 ; 
    p_l_surf = 0x0 ; 
    p_xi_surf = 0x0 ; 
 
}               
 
void Star::del_hydro_euler() {
 
    ener_euler.set_etat_nondef() ; 
    s_euler.set_etat_nondef() ; 
    gam_euler.set_etat_nondef() ; 
    u_euler.set_etat_nondef() ; 
    stress_euler.set_etat_nondef() ;
 
    del_deriv() ; 
 
}               
 
 
 
 
                //--------------//
                //  Assignment  //
                //--------------//
 
// Assignment to another Star
// ----------------------------
void Star::operator=(const Star& et) {
 
    assert( &(et.mp) == &mp ) ;         // Same mapping
    assert( &(et.eos) == &eos ) ;       // Same EOS
    
    nzet = et.nzet ; 
    ent = et.ent ;
    nbar = et.nbar ; 
    ener = et.ener ;
    press = et.press ;
    ener_euler = et.ener_euler ;
    s_euler = et.s_euler ;
    gam_euler = et.gam_euler ;
    u_euler = et.u_euler ;
    stress_euler = et.stress_euler ;
    logn = et.logn ;
    nn = et.nn ;
    beta = et.beta ;
    lnq = et.lnq ;
    gamma = et.gamma ;
 
    del_deriv() ;  // Deletes all derived quantities
 
}   
 
// Assignment of the enthalpy field
// --------------------------------
 
void Star::set_enthalpy(const Scalar& ent_i) {
    
    ent = ent_i ; 
    
    // Update of (nbar, ener, press) :
    equation_of_state() ; 
    
    // The derived quantities are obsolete:
    del_deriv() ; 
    
}
 
                //--------------//
                //    Outputs   //
                //--------------//
 
// Save in a file
// --------------
void Star::sauve(FILE* fich) const {
 
    logn.sauve(fich) ;
    lnq.sauve(fich) ;
  
    int xx = nzet ;     
    fwrite_be(&xx, sizeof(int), 1, fich) ;          
  
    eos.sauve(fich) ; 
    ent.sauve(fich) ;     
}
 
// Printing
// --------
 
ostream& operator<<(ostream& ost, const Star& et)  {
    et >> ost ;
    return ost ;
}
    
ostream& Star::operator>>(ostream& ost) const {
    
  using namespace Unites ;
 
    ost << endl ; 
      
    ost << "Number of domains occupied by the star : " << nzet << endl ; 
    
    ost << "Equation of state : " << endl ; 
    ost << eos << endl ; 
    
    ost << endl << "Central enthalpy : " << ent.val_grid_point(0,0,0,0) << " c^2" << endl ; 
    ost << "Central proper baryon density : " << nbar.val_grid_point(0,0,0,0) 
    << " x 0.1 fm^-3" << endl ; 
    ost << "Central proper energy density : " << ener.val_grid_point(0,0,0,0) 
    << " rho_nuc c^2" << endl ; 
    ost << "Central pressure : " << press.val_grid_point(0,0,0,0) 
    << " rho_nuc c^2" << endl ; 
    
    ost << endl ;
    ost << "Central lapse N :      " << nn.val_grid_point(0,0,0,0) <<  endl ; 
//    ost << "Central value of lnq : " << lnq.val_grid_point(0,0,0,0) <<  endl ; 
  
    ost << endl 
    << "Coordinate equatorial radius (phi=0) a1 =    " 
    << ray_eq()/km << " km" << endl ;  
    ost << "Coordinate equatorial radius (phi=pi/2) a2 = " 
    << ray_eq_pis2()/km << " km" << endl ;  
    ost << "Coordinate equatorial radius (phi=pi):       " 
    << ray_eq_pi()/km << " km" << endl ;  
    ost << "Coordinate polar radius a3 =                 " 
    << ray_pole()/km << " km" << endl ;  
    ost << "Axis ratio a2/a1 = " << ray_eq_pis2() / ray_eq() 
    << "  a3/a1 = " << ray_pole() / ray_eq() << endl ;  
    ost << endl << "Baryon mass :        " << mass_b() / msol << " M_sol" << endl ; 
    ost << "Gravitational mass : " << mass_g() / msol << " M_sol" << endl ; 
    
 
    return ost ; 
}
 
        //-----------------------------------------//
        //  Computation of hydro quantities    //
        //-----------------------------------------//
 
void Star::equation_of_state() {
 
    Scalar ent_eos = ent ;
 
 
    // Slight rescale of the enthalpy field in case of 2 domains inside the
    //  star
 
 
        double epsilon = 1.e-12 ;
 
    const Mg3d* mg = mp.get_mg() ;
        int nz = mg->get_nzone() ;
 
        Mtbl xi(mg) ;
        xi.set_etat_qcq() ;
        for (int l=0; l<nz; l++) {
            xi.t[l]->set_etat_qcq() ;
            for (int k=0; k<mg->get_np(l); k++) {
                for (int j=0; j<mg->get_nt(l); j++) {
                    for (int i=0; i<mg->get_nr(l); i++) {
                        xi.set(l,k,j,i) =
                            mg->get_grille3d(l)->x[i] ;
                    }
                }
            }
 
        }
 
        Scalar fact_ent(mp) ;
        fact_ent.allocate_all() ;
        
        fact_ent.set_domain(0) = 1 + epsilon * xi(0) * xi(0) ;
        fact_ent.set_domain(1) = 1 - 0.25 * epsilon * (xi(1) - 1) * (xi(1) - 1) ;
        
        for (int l=nzet; l<nz; l++) {
            fact_ent.set_domain(l) = 1 ;
        }
 
    if (nzet > 1) {
 
      if(nzet == 3) {
    fact_ent.set_domain(1) = 1 - 0.5 * epsilon * (xi(1) - 0.5) * (xi(1) - 0.5) ;
    fact_ent.set_domain(2) = 1 - 0.25 * epsilon * (xi(2) - 1) * (xi(2) - 1) ;
      }
 
        if (nzet > 3) {
        
            cout << "Star::equation_of_state: not ready yet for nzet > 3 !"
                 << endl ;      
        }
 
        ent_eos = fact_ent * ent_eos ;
        ent_eos.std_spectral_base() ;
    }
 
 
 
 
 
    // Call to the EOS (the EOS is called domain by domain in order to
    //          allow for the use of MEos)
 
    Scalar tempo(mp) ;
 
    nbar.set_etat_qcq() ;
    nbar = 0 ;
    for (int l=0; l<nzet; l++) {
 
        Param par ;       // Paramater for multi-domain equation of state
        par.add_int(l) ;
 
        tempo =  eos.nbar_ent(ent_eos, 1, l, &par) ;
 
        nbar = nbar + tempo ;
 
    }
 
    ener.set_etat_qcq() ;
    ener = 0 ;
    for (int l=0; l<nzet; l++) {
 
        Param par ;    // Paramater for multi-domain equation of state
        par.add_int(l) ;
 
        tempo =  eos.ener_ent(ent_eos, 1, l, &par) ;
 
        ener = ener + tempo ;
 
    }
 
    press.set_etat_qcq() ;
    press = 0 ;
    for (int l=0; l<nzet; l++) {
 
        Param par ;     // Paramater for multi-domain equation of state
        par.add_int(l) ;
 
        tempo =  eos.press_ent(ent_eos, 1, l, &par) ;
 
        press = press + tempo ;
 
    }
 
 
    // Set the bases for spectral expansion
    nbar.std_spectral_base() ; 
    ener.std_spectral_base() ; 
    press.std_spectral_base() ; 
 
    // The derived quantities are obsolete
    del_deriv() ; 
    
}
 
void Star::hydro_euler() {
    
    cout << 
    "Star::hydro_euler : hydro_euler must be called via a derived class"
    << endl << " of Star !" << endl ; 
    
    abort() ;        
    
}
}