etoile_eqsph_falloff.C

/*
 * Method of class Etoile to compute a static spherical configuration
 *  with the outer boundary condition at a finite radius
 *
 * (see file etoile.h for documentation).
 *
 */
 
/*
 *   Copyright (c) 2004 Keisuke Taniguchi
 *
 *   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: etoile_eqsph_falloff.C,v 1.3 2016/12/05 16:17:54 j_novak Exp $
 * $Log: etoile_eqsph_falloff.C,v $
 * Revision 1.3  2016/12/05 16:17:54  j_novak
 * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
 *
 * Revision 1.2  2014/10/13 08:52:58  j_novak
 * Lorene classes and functions now belong to the namespace Lorene.
 *
 * Revision 1.1  2004/11/30 20:52:24  k_taniguchi
 * *** empty log message ***
 *
 *
 *
 * $Header: /cvsroot/Lorene/C++/Source/Etoile/etoile_eqsph_falloff.C,v 1.3 2016/12/05 16:17:54 j_novak Exp $
 *
 */
 
// Headers C
#include "math.h"
 
// Headers Lorene
#include "etoile.h"
#include "param.h"
#include "unites.h"     
 
namespace Lorene {
void Etoile::equil_spher_falloff(double ent_c, double precis) {
    
    // Fundamental constants and units
    // -------------------------------
  using namespace Unites ;
    
    // Initializations
    // ---------------
    
    const Mg3d* mg = mp.get_mg() ; 
    int nz = mg->get_nzone() ;      // total number of domains
    
    // Index of the point at phi=0, theta=pi/2 at the surface of the star:
    int l_b = nzet - 1 ; 
    int i_b = mg->get_nr(l_b) - 1 ; 
    int j_b = mg->get_nt(l_b) - 1 ; 
    int k_b = 0 ; 
    
    // Value of the enthalpy defining the surface of the star
    double ent_b = 0 ; 
    
    // Initialization of the enthalpy field to the constant value ent_c :
    
    ent = ent_c ; 
    ent.annule(nzet, nz-1) ; 
    
    
    // Corresponding profiles of baryon density, energy density and pressure
    
    equation_of_state() ; 
    
    // Initial metric 
    a_car = 1 ;      // this value will remain unchanged in the Newtonian case
    beta_auto = 0 ;  // this value will remain unchanged in the Newtonian case
    
 
    // Auxiliary quantities
    // --------------------
    
    // Affine mapping for solving the Poisson equations
    Map_af mpaff(mp);   
        
    Param par_nul   ;    // Param (null) for Map_af::poisson.
 
    Tenseur ent_jm1(mp) ;   // Enthalpy at previous step
    ent_jm1 = 0 ; 
    
    Tenseur source(mp) ; 
    Tenseur logn(mp) ; 
    Tenseur logn_quad(mp) ; 
    logn = 0 ; 
    logn_quad = 0 ; 
 
    Cmp dlogn(mp) ; 
    Cmp dbeta(mp) ; 
    
    double diff_ent = 1 ;     
    int mermax = 200 ;      // Max number of iterations
    
    double alpha_r = 1 ; 
    int k_falloff = 1 ;
 
    //=========================================================================
    //          Start of iteration
    //=========================================================================
 
    for(int mer=0 ; (diff_ent > precis) && (mer<mermax) ; mer++ ) {
 
    cout << "-----------------------------------------------" << endl ;
    cout << "step: " << mer << endl ;
    cout << "alpha_r: " << alpha_r << endl ;
    cout << "diff_ent = " << diff_ent << endl ;    
 
    //-----------------------------------------------------
    // Resolution of Poisson equation for ln(N)
    //-----------------------------------------------------
 
    // Matter part of ln(N)
    // --------------------
    if (relativistic) {
        source = a_car * (ener + 3*press) ;
    }
    else {
        source = nbar ; 
    }
    
    (source.set()).set_dzpuis(4) ; 
    
    source.set_std_base() ;     // Sets the standard spectral bases. 
    
    logn_auto.set_etat_qcq() ; 
 
    mpaff.poisson_falloff(source(), par_nul, logn_auto.set(), k_falloff) ; 
 
    // NB: at this stage logn_auto is in machine units, not in c^2
 
    // Quadratic part of ln(N)
    // -----------------------
 
    if (relativistic) {
        
        mpaff.dsdr(logn(), dlogn) ; 
        mpaff.dsdr(beta_auto(), dbeta) ; 
        
        source = - dlogn * dbeta ; 
              
        logn_quad.set_etat_qcq() ; 
        
        mpaff.poisson_falloff(source(), par_nul, logn_quad.set(),
                  k_falloff) ; 
                
    }
 
    //-----------------------------------------------------
    // Computation of the new radial scale
    //-----------------------------------------------------
 
    // alpha_r (r = alpha_r r') is determined so that the enthalpy
    // takes the requested value ent_b at the stellar surface
    
    double nu_mat0_b  = logn_auto()(l_b, k_b, j_b, i_b) ; 
    double nu_mat0_c  = logn_auto()(0, 0, 0, 0) ; 
 
    double nu_quad0_b  = logn_quad()(l_b, k_b, j_b, i_b) ; 
    double nu_quad0_c  = logn_quad()(0, 0, 0, 0) ; 
 
    double alpha_r2 = ( ent_c - ent_b - nu_quad0_b + nu_quad0_c )
                / ( qpig*(nu_mat0_b - nu_mat0_c) ) ;
 
    alpha_r = sqrt(alpha_r2) ;
    
    // New radial scale
    mpaff.homothetie( alpha_r ) ; 
 
    //--------------------
    // First integral
    //--------------------
 
    // Gravitation potential in units c^2 :
    logn_auto = alpha_r2*qpig * logn_auto ;
    logn = logn_auto + logn_quad ;
 
    // Enthalpy in all space
    double logn_c = logn()(0, 0, 0, 0) ;
    ent = ent_c - logn() + logn_c ;
 
    //---------------------
    // Equation of state
    //---------------------
    
    equation_of_state() ; 
    
    if (relativistic) {
        
        //----------------------------
        // Equation for beta = ln(AN)
        //----------------------------
        
        mpaff.dsdr(logn(), dlogn) ; 
        mpaff.dsdr(beta_auto(), dbeta) ; 
        
        source = 3 * qpig * a_car * press ;
        
        source = source() 
             - 0.5 * (  dlogn * dlogn + dbeta * dbeta ) ;
    
        source.set_std_base() ;   // Sets the standard spectral bases. 
 
        beta_auto.set_etat_qcq() ; 
             
        mpaff.poisson_falloff(source(), par_nul, beta_auto.set(),
                  k_falloff) ; 
        
 
        // Metric coefficient A^2 update
        
        a_car = exp(2*(beta_auto - logn)) ;
        
    }
    
    // Relative difference with enthalpy at the previous step
    // ------------------------------------------------------
    
    diff_ent = norme( diffrel(ent(), ent_jm1()) ) / nzet ; 
 
    // Next step
    // ---------
    
    ent_jm1 = ent ; 
 
 
    }  // End of iteration loop 
    
    //=========================================================================
    //          End of iteration
    //=========================================================================
 
 
    // The mapping is transfered to that of the star:
    // ----------------------------------------------
    mp = mpaff ; 
    
    
    // Sets value to all the Tenseur's of the star
    // -------------------------------------------
    
    // ... hydro 
    ent.annule(nzet, nz-1) ;    // enthalpy set to zero at the exterior of 
                // the star
    ener_euler = ener ; 
    s_euler = 3 * press ;
    gam_euler = 1 ;  
    u_euler = 0 ; 
    
    // ... metric
    nnn = exp( unsurc2 * logn ) ; 
    nnn.set_std_base() ;
    shift = 0 ; 
    a_car.set_std_base() ;
 
    // Info printing
    // -------------
    
    cout << endl 
     << "Characteristics of the star obtained by Etoile::equil_spher_falloff : " 
     << endl 
     << "-------------------------------------------------------------------" 
     << endl ; 
 
    double ray = mp.val_r(l_b, 1., M_PI/2., 0) ; 
    cout << "Coordinate radius  :       " << ray / km << " km" << endl ; 
 
    double rcirc = ray * sqrt( a_car()(l_b, k_b, j_b, i_b) ) ; 
    
    double compact = qpig/(4.*M_PI) * mass_g() / rcirc ; 
 
    cout << "Circumferential radius R : " << rcirc/km  << " km" << endl ;
    cout << "Baryon mass :       " << mass_b()/msol << " Mo" << endl ;
    cout << "Gravitational mass M :  " << mass_g()/msol << " Mo" << endl ;
    cout << "Compacity parameter GM/(c^2 R) : " << compact << endl ;
 
 
    //-----------------
    // Virial theorem
    //-----------------
    
    //... Pressure term
 
    source = qpig * a_car * sqrt(a_car) * s_euler ; 
    source.set_std_base() ;     
    double vir_mat = source().integrale() ; 
    
    //... Gravitational term
 
    Cmp tmp = beta_auto() - logn() ; 
 
    source =  - ( logn().dsdr() * logn().dsdr() 
              - 0.5 * tmp.dsdr() * tmp.dsdr() ) 
            * sqrt(a_car())  ; 
 
    source.set_std_base() ;
 
    double vir_grav = source().integrale() ;
 
    //... Relative error on the virial identity GRV3
    
    double grv3 = ( vir_mat + vir_grav ) / vir_mat ;
 
    cout << "Virial theorem GRV3 : " << endl ; 
    cout << "     3P term    : " << vir_mat << endl ; 
    cout << "     grav. term : " << vir_grav << endl ; 
    cout << "     relative error : " << grv3 << endl ; 
    
}
}