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/*
* Main code for Isolated Horizon in arbitrary gauge
*
*/
/*
* Copyright (c) 2004-2005 Jose Luis Jaramillo
* 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 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 isolhor_C[] = "$Header: /cvsroot/Lorene/Codes/Isol_hor/isolhor.C,v 1.36 2014/10/13 08:53:56 j_novak Exp $" ;
/*
* $Id: isolhor.C,v 1.36 2014/10/13 08:53:56 j_novak Exp $
* $Log: isolhor.C,v $
* Revision 1.36 2014/10/13 08:53:56 j_novak
* Lorene classes and functions now belong to the namespace Lorene.
*
* Revision 1.35 2014/10/06 15:09:44 j_novak
* Modified #include directives to use c++ syntax.
*
* Revision 1.34 2007/01/22 14:49:53 jl_jaramillo
* versions ok for running tests
*
* Revision 1.33 2006/02/22 16:32:14 jl_jaramillo
* dynamical relaxation
*
* Revision 1.32 2005/10/21 16:38:02 jl_jaramillo
* Control of the expansion
*
* Revision 1.31 2005/10/21 16:20:18 jl_jaramillo
* Version for the paper JaramL05
*
* Revision 1.30 2005/09/12 12:34:09 f_limousin
* Compilation Warning - Change of convention for the angular velocity
* Add Berlin boundary condition in the case of binary horizons.
*
* Revision 1.29 2005/06/09 08:09:10 f_limousin
* Implementation of the Kerr-Shild metric
*
* Revision 1.28 2005/04/08 12:14:42 f_limousin
* Dependance in phi.
*
* Revision 1.27 2005/04/08 09:30:53 jl_jaramillo
* Calculation of the expansion and its radial derivative
*
* Revision 1.26 2005/04/06 08:17:09 f_limousin
* Writing of global quantities in resformat.d
*
* Revision 1.25 2005/04/03 19:48:52 f_limousin
* Implementation of set_psi(psi_in).
*
* Revision 1.24 2005/04/02 15:52:05 f_limousin
* New data member nz. Lichnerowicz choice for aquad. Delete function
* compute_ww().
*
* Revision 1.23 2005/03/31 09:46:33 f_limousin
* New functions compute_ww(..) and aa_kerr_ww().
*
* Revision 1.22 2005/03/30 12:08:33 f_limousin
* Implementation of K^{ij} (Eq.(13) Of Sergio (2002)).
*
* Revision 1.21 2005/03/28 19:42:24 f_limousin
* Implement the metric and A^{ij}A_{ij} of Sergio for pertubations
* of Kerr black holes.
*
* Revision 1.20 2005/03/24 16:50:53 f_limousin
* Add parameters solve_shift and solve_psi in par_isol.d and in function
* init_dat(...). Implement Isolhor::kerr_perturb().
*
* Revision 1.19 2005/03/22 13:25:49 f_limousin
* Small changes. The angular velocity and A^{ij} are computed
* with a differnet sign.
*
* Revision 1.18 2005/03/15 19:28:11 f_limousin
* Implement initial data for Kerr black hole in isotropic coordinates.
*
* Revision 1.17 2005/03/09 10:33:31 f_limousin
* Delete functions init_data_b_neumann(...) and init_data_berlin(...)
* --> New parameter solve_lapse in the function init_data(...).
*
* Revision 1.16 2005/03/03 10:18:57 f_limousin
* Addition of the boost in x and z-direction.
* The grid and the mapping are now saved in the output file.
*
* Revision 1.15 2004/12/31 12:30:07 f_limousin
* Change the construction of an Isol_hor and the function sauve(FILE*, bool).
*
* Revision 1.14 2004/11/18 10:02:37 jl_jaramillo
* gamt and gamt_point well constructed as tensor in spaherical
* components
*
* Revision 1.13 2004/11/09 12:40:08 f_limousin
* Add some printing
*
* Revision 1.12 2004/11/05 17:53:26 f_limousin
* Perturbations of the conformal metric and its time derivative.
*
* Revision 1.8 2004/11/02 17:42:00 f_limousin
* New method sauve(...) to save in a binary file.
*
* Revision 1.6 2004/10/29 15:41:02 jl_jaramillo
* ADM angular momentum added
*
* Revision 1.5 2004/10/01 16:48:47 f_limousin
* *** empty log message ***
*
* Revision 1.4 2004/09/28 15:57:45 f_limousin
* Add the 2 lines $Id and $Log to see the comments
*
*
* Revision 1.1 2004/02/18 19:16:28 jl_jaramillo
* First version: c'est loin d'etre pret tout ca !!!
*
*
* $Header: /cvsroot/Lorene/Codes/Isol_hor/isolhor.C,v 1.36 2014/10/13 08:53:56 j_novak Exp $
*
*/
// C++ headers
#include "headcpp.h"
// C headers
#include <cstdlib>
#include <cmath>
#include <cstring>
// Lorene headers
#include "tenseur.h"
#include "metric.h"
#include "evolution.h"
#include "param.h"
#include "nbr_spx.h"
#include "utilitaires.h"
#include "graphique.h"
#include "time_slice.h"
#include "isol_hor.h"
using namespace Lorene ;
int main() {
//======================================================================
// Construction and initialization of the various objects
//======================================================================
// Setup of a multi-domain grid (Lorene class Mg3d)
// ------------------------------------------------
int nz, nt, np, nr1, nrp1 ;
ifstream fpar("par_hor.d") ;
fpar.ignore(1000, '\n') ;
fpar.ignore(1000, '\n') ;
fpar >> nz; fpar.ignore(1000, '\n');
fpar >> nt; fpar.ignore(1000, '\n');
fpar >> np; fpar.ignore(1000, '\n');
fpar >> nr1; fpar.ignore(1000, '\n');
fpar >> nrp1; fpar.ignore(1000, '\n');
int type_t = SYM ; // symmetry with respect to the equatorial plane
int type_p = NONSYM ; // no symmetry in phi
// Reading of the parameter file
// ------------------------------
int niter, bound_nn, bound_psi, bound_beta, solve_lapse, solve_psi ;
int solve_shift ;
double radius, relax_nn, relax_psi, relax_beta, seuil, ang_vel, boost_x, boost_z, lim_nn ;
fpar >> radius; fpar.ignore(1000, '\n');
fpar >> relax_nn; fpar.ignore(1000, '\n');
fpar >> relax_psi; fpar.ignore(1000, '\n');
fpar >> relax_beta; fpar.ignore(1000, '\n');
fpar >> seuil; fpar.ignore(1000, '\n');
fpar >> niter; fpar.ignore(1000, '\n');
fpar >> ang_vel; fpar.ignore(1000, '\n');
fpar >> boost_x ;
fpar >> boost_z; fpar.ignore(1000, '\n');
fpar >> bound_nn ;
fpar >> lim_nn ; fpar.ignore(1000, '\n');
fpar >> bound_psi ; fpar.ignore(1000, '\n');
fpar >> bound_beta ; fpar.ignore(1000, '\n');
fpar >> solve_lapse ; fpar.ignore(1000, '\n');
fpar >> solve_psi ; fpar.ignore(1000, '\n');
fpar >> solve_shift ; fpar.ignore(1000, '\n');
int* nr_tab = new int[nz];
int* nt_tab = new int[nz];
int* np_tab = new int[nz];
double* bornes = new double[nz+1];
for (int l=0; l<nz; l++) {
if (l==1) nr_tab[1] = nr1 ;
else nr_tab[l] = nrp1 ;
np_tab[l] = np ;
nt_tab[l] = nt ;
bornes[l] = pow(2., l-1) * radius ;
}
bornes[0] = 0. ;
bornes[nz] = __infinity ;
// Type of r sampling :
int* type_r = new int[nz];
type_r[0] = RARE ;
for (int l=1; l<nz-1; l++) {
type_r[l] = FIN ;
}
type_r[nz-1] = UNSURR ;
// Multi-domain grid construction:
Mg3d mgrid(nz, nr_tab, type_r, nt_tab, type_t, np_tab, type_p) ;
Map_af mp(mgrid, bornes) ; // Mapping construction
// Denomination of various coordinates associated with the mapping
// ---------------------------------------------------------------
const Coord& r = mp.r ; // r field
const Coord& theta = mp.tet ; // r field
const Coord& costt = mp.cost ; // cos(theta) field
const Coord& sintt = mp.sint ; // sin(theta) field
const Coord& cospp = mp.cosp ; // cos(phi) field
const Coord& sinpp = mp.sinp ; // sin(phi) field
Scalar rr(mp) ;
rr = r ;
rr.std_spectral_base() ;
Scalar cos2t (mp) ;
cos2t = cos(2.*theta) ;
Scalar cost (mp) ;
cost = costt ;
Scalar cosp (mp) ;
cosp = cospp ;
Scalar sint (mp) ;
sint = sintt ;
Scalar sinp (mp) ;
sinp = sinpp ;
// Flat metric f
// -------------
const Metric_flat& ff = mp.flat_met_spher() ;
const Base_vect_spher& otriad = mp.get_bvect_spher() ;
// Working stuff
// -------------
Scalar tmp_scal(mp) ;
Vector tmp_vect(mp, CON, otriad) ;
Sym_tensor tmp_sym(mp, CON, otriad) ;
// Key function
Scalar unsr(1./rr) ;
unsr.set_domain(0) = 1 ; // scalar set to 1 in the nucleus
unsr.std_spectral_base() ;
Scalar expmr (exp (- 1/((rr-1)*(rr-1)))) ;
expmr.std_spectral_base() ;
Scalar expmrr (exp(-pow(rr-3,2.))) ;
expmrr.std_spectral_base() ;
// =================================================================
// =================================================================
// Physical Parameters
//--------------------
// Set up of lapse function N
// --------------------------
Scalar nn_init(mp) ;
nn_init = 1. - 0.5*unsr ;
nn_init.std_spectral_base() ; // sets standard spectral bases
// Set up of field Psi
// -------------------
Scalar psi_init(mp) ;
psi_init = 1. ;
psi_init.std_spectral_base() ; // sets standard spectral bases
// Set up of shift vector beta
// ---------------------------
Vector beta_init(mp, CON, mp.get_bvect_spher()) ;
beta_init.set(1) = 0.2*unsr*unsr ;
beta_init.set(2) = 0. ;
beta_init.set(3) = 0. ;
beta_init.annule_domain(0) ;
beta_init.std_spectral_base() ;
// TrK, TrK_point
// --------------
Scalar trK (mp) ;
trK = 0.*unsr*unsr*unsr*unsr ;
trK.std_spectral_base() ;
trK.inc_dzpuis(2) ;
Scalar trK_point (mp) ;
trK_point = 0. ;
trK_point.std_spectral_base() ;
trK_point.inc_dzpuis(2) ;
// gamt, gamt_point
// ----------------
Scalar khi (mp) ;
khi = 0.0 *unsr*unsr*sint*sint*sinp*cosp ;
khi.std_spectral_base() ;
khi.annule_domain(0) ;
// cout << "khi : " << endl ;
// cout << khi << endl ;
Scalar mu (mp) ;
mu = 0.0*unsr*unsr*cost ;
mu.set_spectral_va().set_base_r(0,R_CHEBPIM_P) ;
for (int i=1 ; i<nz-1 ; i++){
mu.set_spectral_va().set_base_r(i,R_CHEB) ;
}
mu.set_spectral_va().set_base_r(nz-1,R_CHEBU) ;
mu.set_spectral_va().set_base_t(T_COSSIN_CI) ;
mu.set_spectral_va().set_base_p(P_COSSIN) ;
mu.annule_domain(0) ;
Sym_tensor_tt hh_tmp (mp, otriad, ff) ;
hh_tmp.set_khi_mu(khi, mu) ;
//Construction of a gamt
//----------------------
Sym_tensor gamt(mp, COV, mp.get_bvect_spher()) ;
gamt = ff.cov() + hh_tmp.up_down(ff) ;
cout << gamt << endl ;
/*
gamt.set(1,1) = gamt(1,1) * (1+0.3*sint*sint*cosp*cosp*
(1/rr/rr - 1/rr/rr/rr)) ;
gamt.set(2,2) = gamt(2,2) * (1+0.01*sint*sint*cosp*cosp*
(1/rr/rr - 1/rr/rr/rr)) ;
gamt.set(3,3) = gamt(3,3) * (1+0.01*sint*sint*cosp*cosp*
(1/rr/rr - 1/rr/rr/rr)) ;
gamt.set(1,3) = 0.1*sint*sint*cosp*(1/rr/rr - 1/rr/rr/rr) ;
gamt.set(1,3).set_spectral_va().set_base_t(T_COSSIN_SI) ;
*/
gamt.std_spectral_base() ;
// Determinant of gamma tilde is put to one
// ----------------------------------------
Metric met_gamt_tmp (gamt) ;
Scalar det_ust = pow(met_gamt_tmp.determinant(), -1./3.) ;
det_ust.std_spectral_base() ;
gamt = gamt*det_ust ;
Metric met_gamt (gamt) ;
// Gamma-tilde_point
//------------------
khi = 0. ;
khi.std_spectral_base() ;
mu = 0. ;
mu.std_spectral_base() ;
hh_tmp.set_khi_mu(khi, mu) ;
Sym_tensor gamt_point(mp, CON, mp.get_bvect_spher()) ;
gamt_point = hh_tmp ;
gamt_point.inc_dzpuis(2) ;
// =================================================================
// =================================================================
double mm, aaa, hh ;
/*
//--------------------------------------------------
// Construction of Kerr Metric
//--------------------------------------------------
Scalar a2(mp) ;
Scalar b2(mp) ;
// Parameters
// -----------
hh = 2. ;
double jj = 0. ;
aaa = - pow( 0.5*(pow(hh*hh*hh*hh+4.*jj*jj, 0.5) - hh*hh), 0.5) ;
mm = pow(aaa*aaa + hh*hh, 0.5) ;
a2 = 1. + 2.*mm/rr + (3.*mm*mm + aaa*aaa*cos2t)/(2.*rr*rr)
+ (hh*hh*mm)/(2.*pow(rr, 3.)) + pow(hh,4.)/(16.*pow(rr,4.)) ;
a2.std_spectral_base() ;
a2.set_domain(0) = 1. ;
b2 = ( pow(rr,8.) + 4.*mm*pow(rr,7.) + (7.*mm*mm +
aaa*aaa*cost*cost)*pow(rr,6.) + mm*(7.*mm*mm+aaa*aaa)
*pow(rr,5.) + (4.*pow(mm,4.) + hh*hh*(3.*hh*hh/4.+aaa*aaa*sint
*sint)/2.)*pow(rr,4.) + hh*hh*mm*(2.*mm*mm-hh*hh/4.)
*pow(rr,3.) + pow(hh,4.)/16.*(7.*mm*mm + aaa*aaa*cost
*cost)*rr*rr + pow(hh,6.)*mm/16.*rr + pow(hh,8.)/256. )
/ ( pow(rr,8.) + 2.*mm*pow(rr,7.) + (3.*mm*mm + aaa*aaa
*cos2t)/2.*pow(rr,6.) + hh*hh*mm/2.*pow(rr,5.)
+ pow(hh,4.)/16.*pow(rr,4.)) ;
b2.set_outer_boundary(nz-1 ,1.) ;
b2.std_spectral_base() ;
b2.set_domain(0) = 1. ;
// Construction of the tilde metric
// ---------------------------------
Sym_tensor h_uu(mp, CON, mp.get_bvect_spher()) ;
for (int i=1; i<=3; i++)
for (int j=1; j<=i; j++){
if(i != j){
h_uu.set(i,j) = 0. ;
}
}
h_uu.set(1,1) = pow(b2/a2, 1./3.) - 1 ;
h_uu.set(2,2) = pow(b2/a2, 1./3.) - 1 ;
h_uu.set(3,3) = pow(a2/b2, 2./3.) - 1 ;
h_uu.annule_domain(0) ;
h_uu.std_spectral_base() ;
// Metric tgam (ff.con() + h_uu) ;
Metric tgam (ff.con()) ; //For computing BY and DainLT
gamt = tgam.cov() ;
met_gamt = gamt ;
// Determinant of gamma tilde is put to one
// ----------------------------------------
met_gamt_tmp = met_gamt ;
det_ust = pow(met_gamt_tmp.determinant(), -1./3.) ;
det_ust.std_spectral_base() ;
gamt = gamt*det_ust ;
met_gamt = gamt ;
cout << "norme de gamt" << endl << norme(gamt(1,1)) << endl
<< norme(gamt(2,1)) << endl << norme(gamt(3,1)) << endl
<< norme(gamt(2,2)) << endl << norme(gamt(3,2)) << endl
<< norme(gamt(3,3)) << endl ;
// Angular velocity
// ----------------
ang_vel = -1.*aaa / (2*mm*(mm+pow(mm*mm-aaa*aaa, 0.5))) ;
cout << "ang_vel = " << ang_vel << endl ;
// Lapse function
// --------------
Scalar nnn (mp) ;
nnn = ( pow(rr, 8) + 2*mm*pow(rr, 7) + (mm*mm+aaa*aaa*cost
*cost)*pow(rr, 6)
- 0.5*hh*hh*mm*pow(rr, 5) - 0.5*hh*hh*(mm*mm+0.25*hh*hh
+aaa*aaa*cost*cost)*pow(rr,4)
- pow(hh,4)*mm/8.*rr*rr*rr + pow(hh,4)/16.*(mm*mm +
aaa*aaa*cost*cost)*rr*rr + pow(hh,6)*mm/32.*rr
+ pow(hh,8)/256.) / (pow(rr,8) + 4*mm*pow(rr,7)
+ (7*mm*mm+aaa*aaa*cost*cost)*pow(rr,6)
+ mm*(7*mm*mm+aaa*aaa)*pow(rr,5) + (4*mm*mm*mm*mm
+ 0.5*hh*hh*(0.75*hh*hh+aaa*aaa*sint*sint))*pow(rr,4)
+ hh*hh*mm*(2*mm*mm-0.25*hh*hh)*pow(rr,3)
+ pow(hh,4)/16.*(7*mm*mm+aaa*aaa*cost*cost)*rr*rr
+ pow(hh,6)*mm/16.*rr + pow(hh,8)/256.) ;
nnn.std_spectral_base() ;
if (bound_nn == 5 && solve_lapse == 1)
nnn = pow(nnn, 0.5) + 0.2*unsr*unsr ;
else
nnn = pow(nnn, 0.5) + 0.2*unsr*unsr ;
nnn.set_outer_boundary(nz-1 ,1.) ;
if (bound_nn == 5 && solve_lapse == 1)
nnn.set_inner_boundary(1, 0.2) ;
else
nnn.set_inner_boundary(1, 0.2) ;
nnn.set_domain(0) = 1. ;
nnn.std_spectral_base() ;
nn_init = nnn ;
// Shift vector
// ------------
Scalar beta_phi (mp) ;
beta_phi = 2*aaa*mm*unsr*unsr*sint/(a2*b2)
*(1+mm*unsr+0.25*hh*hh*unsr*unsr) ;
beta_phi.std_spectral_base() ;
beta_phi.set_domain(0) = 0. ;
Vector beta_kerr (mp, CON, mp.get_bvect_spher()) ;
beta_kerr.set(1) = 0.0*unsr*unsr ;
beta_kerr.set(2) = 0. ;
beta_kerr.set(3) = beta_phi ;
beta_kerr.std_spectral_base() ;
beta_init = beta_kerr ;
// Conformal factor Psi
// ---------------------
Scalar psi_kerr (pow(a2, 1./6.) * pow(b2,1./12.)) ;
psi_kerr.std_spectral_base() ;
psi_kerr.set_domain(0) = 1. ;
psi_init = psi_kerr ;
// --------------------------------------
// End of the setup of Kerr metric
// --------------------------------------
*/
// Set up of extrinsic curvature
// -----------------------------
Metric met_gam(psi_init*psi_init*psi_init*psi_init*gamt) ;
Sym_tensor kk_init (mp, CON, mp.get_bvect_spher()) ;
int check ;
check = 0 ;
for (int k=0; k<np_tab[1]; k++)
for (int j=0; j<nt_tab[1]; j++){
if (nn_init.val_grid_point(1, k, j , 0) < 1e-12){
check = 1 ;
break ;
}
}
if (check == 0)
kk_init = - 0.5 * met_gam.con().derive_lie(beta_init) / nn_init ;
else {
Sym_tensor kk_temp (mp, CON, mp.get_bvect_spher()) ;
kk_temp = - 0.5 * met_gam.con().derive_lie(beta_init) ;
Scalar nn_sxpun (division_xpun (Cmp(nn_init), 0)) ;
nn_sxpun.set_domain(0) = 1. ;
Scalar auxi (mp) ;
for (int i=1 ; i<=3 ; i++)
for (int j=i ; j<=3 ; j++) {
auxi = kk_temp(i, j) ;
auxi.annule_domain(0) ;
auxi = division_xpun (auxi, 0) ;
kk_init.set(i,j) = auxi / nn_sxpun ;
}
}
Sym_tensor aa_init (mp, CON, mp.get_bvect_spher()) ;
aa_init = psi_init*psi_init*psi_init*psi_init*kk_init
- 1./3. * trK * met_gamt.con() ;
//-------------------------------------
// Construction of the space-time
//-------------------------------------
cout << met_gamt << endl ;
Isol_hor isolhor(mp, nn_init, psi_init, beta_init, aa_init, met_gamt,
gamt_point, trK, trK_point, ff, 3) ;
// In order to initialise isolhor.k_uu() and k_dd() at the good value
Sym_tensor bidon (mp, CON, mp.get_bvect_spher()) ;
bidon = isolhor.k_uu() ;
Sym_tensor bidon2 (isolhor.k_dd()) ;
Scalar bidon3 (isolhor.aa_quad()) ;
//-------------------------------------------------------
// Test of the formula for A^{ij}A_{ij} in Sergio's paper
//-------------------------------------------------------
//isolhor.aa_kerr_ww(mm, aaa) ;
// New initialisation of the metric quantities
// --------------------------------------------
//psi_init = 0.9*psi_kerr ;
// psi_init.std_spectral_base() ;
// isolhor.set_psi(psi_init) ;
// nn_init = 1. ;
// nn_init.std_spectral_base() ;
// Test of the constraints
//------------------------
cout<< "----------------------------------------" <<endl ;
isolhor.check_hamiltonian_constraint() ;
isolhor.check_momentum_constraint() ;
cout<< "----------------------------------------" <<endl ;
//-----------------------------------------
// "Call to init_data.C"
//-----------------------------------------
isolhor.set_omega(ang_vel) ;
isolhor.set_boost_x(boost_x) ;
isolhor.set_boost_z(boost_z) ;
isolhor.init_data(bound_nn, lim_nn, bound_psi, bound_beta, solve_lapse,
solve_psi, solve_shift, seuil, relax_nn, relax_psi, relax_beta, niter) ;
// isolhor.init_data_CTS_gen(bound_nn, lim_nn, bound_psi, bound_beta, solve_lapse,
// solve_psi, solve_shift, seuil, relax_nn, relax_psi, relax_beta, niter, -1., 4.) ;
// Expansion
//----------
Scalar expansion = contract(isolhor.gam().radial_vect().derive_cov(isolhor.gam()), 0,1)
+ contract(contract(isolhor.k_dd(), 0, isolhor.gam().radial_vect(), 0),
0, isolhor.gam().radial_vect(), 0)
- isolhor.trk() ;
double der_expansion_0 = expansion.derive_cov(isolhor.gam())(1)
.val_point(1.00000001, 0, 0.) ;
double der_expansion_1 = expansion.derive_cov(isolhor.gam())(1)
.val_point(1.00000001, M_PI/4, 0.) ;
double der_expansion_2 = expansion.derive_cov(isolhor.gam())(1)
.val_point(1.00000001, M_PI/2, 0.) ;
cout << "Radial derivative of the expansion at (1,0,0) = "
<< der_expansion_0<<endl ;
cout << "Radial derivative of the expansion at (1,Pi/4,0) = "
<< der_expansion_1<<endl ;
cout << "Radial derivative of the expansion at (1,Pi/2,0) = "
<< der_expansion_2<<endl ;
cout << "------------------------------------------------------"<<endl;
/*
des_meridian(expansion, 1, 1.2, "Expansion theta", 2) ;
des_meridian(expansion, 1, 4., "Expansion theta", 1) ;
des_meridian(expansion, 1, 10., "Expansion theta", 3) ;
arrete() ;
*/
double max_exp = expansion.val_grid_point(1, 0, 0, 0) ;
double min_exp = expansion.val_grid_point(1, 0, 0, 0) ;
int nnp = mp.get_mg()->get_np(1) ;
int nnt = mp.get_mg()->get_nt(1) ;
for (int k=0 ; k<nnp ; k++)
for (int j=0 ; j<nnt ; j++){
if (expansion.val_grid_point(1, k, j, 0) > max_exp)
max_exp = expansion.val_grid_point(1, k, j, 0) ;
if (expansion.val_grid_point(1, k, j, 0) < min_exp)
min_exp = expansion.val_grid_point(1, k, j, 0) ;
}
cout << "max_exp = " << max_exp << endl
<< "min_exp = " << min_exp << endl ;
// Save in a file
// --------------
FILE* fresu = fopen("resu.d", "w") ;
mgrid.sauve(fresu) ;
mp.sauve(fresu) ;
isolhor.sauve(fresu, true) ;
fclose(fresu) ;
// Test of the constraints
//------------------------
if (solve_shift == 1)
isolhor.update_aa() ;
else
isolhor.aa_kerr_ww(mm, aaa) ;
cout<< "----------------------------------------" <<endl ;
Tbl check_ham = isolhor.check_hamiltonian_constraint() ;
Tbl check_mom = isolhor.check_momentum_constraint() ;
cout<< "----------------------------------------" <<endl ;
// Physical parameters of the Black Hole
//--------------------------------------
cout<< "------------------------------------------------" <<endl;
cout<< " Physical parameters of the Black Hole " <<endl;
cout<< "------------------------------------------------" <<endl;
double rr_hor = isolhor.radius_hor() ;
cout<< "Radius of the horizon = " << rr_hor <<endl ;
double jj_hor = isolhor.ang_mom_hor() ;
cout<< "Angular momentum of the horizon = " << jj_hor <<endl ;
double mm_hor = isolhor.mass_hor() ;
cout<< "Mass of the horizon = " << mm_hor <<endl ;
double kappa_hor = isolhor.kappa_hor() ;
cout<< "Surface gravity of the horizon = " << kappa_hor <<endl ;
double omega_hor = isolhor.omega_hor() ;
cout<< "Orbital velocity of the horizon = " << omega_hor <<endl ;
// Physical parameters of the Bulk
//--------------------------------
cout.precision(8) ;
cout<< endl;
cout<< "------------------------------------------------" <<endl;
cout<< " Physical parameters of the Bulk " <<endl;
cout<< "------------------------------------------------" <<endl;
double mm_adm = isolhor.adm_mass() ;
cout << "ADM mass= " << mm_adm <<endl ;
double jj_adm = isolhor.ang_mom_adm() ;
cout << "ADM angular momentum= " << jj_adm <<endl ;
double aa = jj_adm / mm_adm ;
cout << "J / M (ADM) : " << aa << endl ;
double aasmm = aa / mm_adm ;
cout << "J / M^2 : " << aasmm << endl ;
double epsa = isolhor.area_hor() /
(8*M_PI*(mm_adm*mm_adm + pow(pow(mm_adm, 4.) - jj_adm*jj_adm, 0.5))) ;
cout << "epsilon A : " << epsa << endl ;
double diff_mm = (mm_adm - mm_hor) / mm_adm ;
cout << "diff mass : " << diff_mm << endl ;
double diff_jj = (jj_adm - jj_hor) / jj_adm ;
cout << "diffangular momentum : " << diff_jj << endl ;
// Writing of all global quantities in a file
ofstream resformat("resformat.d") ;
resformat.precision(6) ;
resformat << "# Ham. constr. Mom. constr. " << endl ;
resformat << max(check_ham) << " " << max(check_mom) << endl ;
resformat.precision(10) ;
resformat << "# r_hor J_hor M_hor kappa_hor omega_hor" << endl ;
resformat << rr_hor << " " << jj_hor << " " << mm_hor << " "
<< kappa_hor << " " << omega_hor << endl ;
resformat << "# M_adm J_adm J/M J/M2 Eps_a" << endl ;
resformat << mm_adm << " " << jj_adm << " " << aa << " "
<< aasmm << " " << epsa << endl ;
resformat << "# diff_mm diff_jj" << endl ;
resformat << diff_mm << " " << diff_jj << endl ;
resformat.close() ;
//--------------------------------------
// Comparison
//--------------------------------------
cout<<"Tout va bien boudiou / Todo bien!!! (Viva Cai!)"<<endl ;
return EXIT_SUCCESS ;
}
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