LORENE
star_bhns_equilibrium.C
1 /*
2  * Method of class Star_bhns to compute an equilibrium configuration
3  * of a neutron star in a black hole-neutron star binary
4  *
5  * (see file star_bhns.h for documentation).
6  *
7  */
8 
9 /*
10  * Copyright (c) 2005-2007 Keisuke Taniguchi
11  *
12  * This file is part of LORENE.
13  *
14  * LORENE is free software; you can redistribute it and/or modify
15  * it under the terms of the GNU General Public License version 2
16  * as published by the Free Software Foundation.
17  *
18  * LORENE is distributed in the hope that it will be useful,
19  * but WITHOUT ANY WARRANTY; without even the implied warranty of
20  * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
21  * GNU General Public License for more details.
22  *
23  * You should have received a copy of the GNU General Public License
24  * along with LORENE; if not, write to the Free Software
25  * Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA
26  *
27  */
28 
29 
30 
31 /*
32  * $Id: star_bhns_equilibrium.C,v 1.6 2018/11/16 14:34:37 j_novak Exp $
33  * $Log: star_bhns_equilibrium.C,v $
34  * Revision 1.6 2018/11/16 14:34:37 j_novak
35  * Changed minor points to avoid some compilation warnings.
36  *
37  * Revision 1.5 2016/12/05 16:18:16 j_novak
38  * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
39  *
40  * Revision 1.4 2014/10/13 08:53:40 j_novak
41  * Lorene classes and functions now belong to the namespace Lorene.
42  *
43  * Revision 1.3 2014/10/06 15:13:16 j_novak
44  * Modified #include directives to use c++ syntax.
45  *
46  * Revision 1.2 2008/05/15 19:13:45 k_taniguchi
47  * Change of some parameters.
48  *
49  * Revision 1.1 2007/06/22 01:30:45 k_taniguchi
50  * *** empty log message ***
51  *
52  *
53  * $Header: /cvsroot/Lorene/C++/Source/Star_bhns/star_bhns_equilibrium.C,v 1.6 2018/11/16 14:34:37 j_novak Exp $
54  *
55  */
56 
57 // C++ headers
58 //#include <>
59 
60 // C headers
61 #include <cmath>
62 
63 // Lorene headers
64 #include "star_bhns.h"
65 #include "param.h"
66 #include "cmp.h"
67 #include "tenseur.h"
68 #include "utilitaires.h"
69 #include "unites.h"
70 //#include "graphique.h"
71 
72 namespace Lorene {
73 void Star_bhns::equilibrium_bhns(double ent_c, const double& mass_bh,
74  const double& sepa, bool kerrschild,
75  int, int mermax_ns, int mermax_potvit,
76  int mermax_poisson, int filter_r,
77  int filter_r_s, int filter_p_s,
78  double relax_poisson, double relax_potvit,
79  double thres_adapt, double resize_ns,
80  const Tbl& fact_resize, Tbl& diff) {
81 
82  // Fundamental constants and units
83  // -------------------------------
84  using namespace Unites ;
85 
86  // Initializations
87  // ---------------
88 
89  const Mg3d* mg = mp.get_mg() ;
90  int nz = mg->get_nzone() ; // Total number of domain
91  // int nt = mg->get_nt(0) ;
92 
93  // The following is required to initialize mp_prev as a Map_et:
94  Map_et& mp_et = dynamic_cast<Map_et&>(mp) ;
95 
96  // Domain and radial indices of points at the surface of the star:
97  int l_b = nzet - 1 ;
98  int i_b = mg->get_nr(l_b) - 1 ;
99  int k_b ;
100  int j_b ;
101 
102  // Value of the enthalpy defining the surface of the star
103  double ent_b = 0 ;
104 
105  // Error indicators
106  // ----------------
107 
108  double& diff_ent = diff.set(0) ;
109  double& diff_vel_pot = diff.set(1) ;
110  double& diff_lapconf = diff.set(2) ;
111  double& diff_confo = diff.set(3) ;
112  double& diff_shift_x = diff.set(4) ;
113  double& diff_shift_y = diff.set(5) ;
114  double& diff_shift_z = diff.set(6) ;
115  double& diff_dHdr = diff.set(7) ;
116  double& diff_dHdr_min = diff.set(8) ;
117  double& diff_phi_min = diff.set(9) ;
118  double& diff_radius = diff.set(10) ;
119 
120  // Parameters for the function Map_et::adapt
121  // -----------------------------------------
122 
123  Param par_adapt ;
124  int nitermax = 100 ;
125  int niter ;
126  int adapt_flag = 1 ; // 1 = performs the full computation,
127  // 0 = performs only the rescaling by
128  // the factor alpha_r
129 
130  // Number of domains for searching the enthalpy isosurfaces
131  int nz_search = nzet + 1 ;
132  // int nz_search = nzet ;
133 
134  double precis_secant = 1.e-14 ;
135  double alpha_r ;
136  double reg_map = 1. ; // 1 = regular mapping, 0 = contracting mapping
137 
138  Tbl ent_limit(nz) ;
139 
140  par_adapt.add_int(nitermax, 0) ; // maximum number of iterations to
141  // locate zeros by the secant method
142  par_adapt.add_int(nzet, 1) ; // number of domains where the
143  // adjustment to the isosurfaces of
144  // ent is to be performed
145  par_adapt.add_int(nz_search, 2) ; // number of domains to search for
146  // the enthalpy isosurface
147  par_adapt.add_int(adapt_flag, 3) ; // 1 = performs the full computation,
148  // 0 = performs only the rescaling by
149  // the factor alpha_r
150  par_adapt.add_int(j_b, 4) ; // theta index of the collocation point
151  // (theta_*, phi_*)
152  par_adapt.add_int(k_b, 5) ; // theta index of the collocation point
153  // (theta_*, phi_*)
154  par_adapt.add_int_mod(niter, 0) ; // number of iterations actually used
155  // in the secant method
156  par_adapt.add_double(precis_secant, 0) ; // required absolute precision in
157  // the determination of zeros by
158  // the secant method
159  par_adapt.add_double(reg_map, 1) ; // 1. = regular mapping,
160  // 0 = contracting mapping
161  par_adapt.add_double(alpha_r, 2) ; // factor by which all the radial
162  // distances will be multiplied
163  par_adapt.add_tbl(ent_limit, 0) ; // array of values of the field ent
164  // to define the isosurfaces
165 
166  Cmp ssjm1lapconf(ssjm1_lapconf) ;
167  Cmp ssjm1confo(ssjm1_confo) ;
168 
169  ssjm1lapconf.set_etat_qcq() ;
170  ssjm1confo.set_etat_qcq() ;
171 
172  double precis_poisson = 1.e-14 ;
173 
174  // Parameters for the function Scalar::poisson for lapconf_auto
175  // ------------------------------------------------------------
176 
177  Param par_lapconf ;
178 
179  par_lapconf.add_int(mermax_poisson, 0) ; // maximum number of iterations
180  par_lapconf.add_double(relax_poisson, 0) ; // relaxation parameter
181  par_lapconf.add_double(precis_poisson, 1) ; // required precision
182  par_lapconf.add_int_mod(niter, 0) ; // number of iterations actually used
183  par_lapconf.add_cmp_mod( ssjm1lapconf ) ;
184 
185  // Parameters for the function Scalar::poisson for confo_auto
186  // ----------------------------------------------------------
187 
188  Param par_confo ;
189 
190  par_confo.add_int(mermax_poisson, 0) ; // maximum number of iterations
191  par_confo.add_double(relax_poisson, 0) ; // relaxation parameter
192  par_confo.add_double(precis_poisson, 1) ; // required precision
193  par_confo.add_int_mod(niter, 0) ; // number of iterations actually used
194  par_confo.add_cmp_mod( ssjm1confo ) ;
195 
196  // Parameters for the function Vector::poisson for shift method 2
197  // --------------------------------------------------------------
198 
199  Param par_shift2 ;
200 
201  par_shift2.add_int(mermax_poisson, 0) ; // maximum number of iterations
202  par_shift2.add_double(relax_poisson, 0) ; // relaxation parameter
203  par_shift2.add_double(precis_poisson, 1) ; // required precision
204  par_shift2.add_int_mod(niter, 0) ; // number of iterations actually used
205 
206  Cmp ssjm1khi(ssjm1_khi) ;
207  ssjm1khi.set_etat_qcq() ;
208 
209  Tenseur ssjm1wshift(mp, 1, CON, mp.get_bvect_cart()) ;
210  ssjm1wshift.set_etat_qcq() ;
211  for (int i=0; i<3; i++) {
212  ssjm1wshift.set(i) = Cmp(ssjm1_wshift(i+1)) ;
213  }
214 
215  par_shift2.add_cmp_mod(ssjm1khi) ;
216  par_shift2.add_tenseur_mod(ssjm1wshift) ;
217 
218  Scalar ent_jm1 = ent ; // Enthalpy at previous step
219 
220  Scalar lapconf_m1(mp) ; // = lapconf_auto - 0.5
221  Scalar confo_m1(mp) ; // = confo_auto - 0.5
222 
223  Scalar source_lapconf(mp) ; // Source term in the equation for lapconf_auto
224  source_lapconf.set_etat_qcq() ;
225  Scalar source_confo(mp) ; // Source term in the equation for confo_auto
226  source_confo.set_etat_qcq() ;
227  Vector source_shift(mp, CON, mp.get_bvect_cart()) ; // Source term
228  // in the equation for shift_auto
229  source_shift.set_etat_qcq() ;
230 
231  //===========================================================
232  // Start of iteration
233  //===========================================================
234 
235  for (int mer_ns=0; mer_ns<mermax_ns; mer_ns++) {
236 
237  cout << "-----------------------------------------------" << endl ;
238  cout << "step: " << mer_ns << endl ;
239  cout << "diff_ent = " << diff_ent << endl ;
240 
241  //------------------------------------------------------
242  // Resolution of the elliptic equation for the velocity
243  // scalar potential
244  //------------------------------------------------------
245 
246  if (irrotational) {
247  diff_vel_pot = velo_pot_bhns(mass_bh, sepa, kerrschild,
248  mermax_potvit, precis_poisson,
249  relax_potvit) ;
250  }
251  else {
252  diff_vel_pot = 0. ; // to avoid the warning
253  }
254 
255  //-------------------------------------
256  // Computation of the new radial scale
257  //-------------------------------------
258 
259  // alpha_r (r = alpha_r r') is determined so that the enthalpy
260  // takes the requested value ent_b at the stellar surface
261 
262  // Values at the center of the star:
263  // lapconf_auto = lapconf_auto=0(r->infty) + 0.5
264  // The term lapconf_auto=0(r->infty) should be rescaled.
265  double lapconf_auto_c = lapconf_auto.val_grid_point(0,0,0,0) - 0.5 ;
266  double lapconf_comp_c = lapconf_comp.val_grid_point(0,0,0,0) ;
267 
268  double confo_c = confo_tot.val_grid_point(0,0,0,0) ;
269 
270  double gam_c = gam.val_grid_point(0,0,0,0) ;
271  double gam0_c = gam0.val_grid_point(0,0,0,0) ;
272 
273  double hhh_c = exp(ent_c) ;
274  double hhh_b = exp(ent_b) ;
275 
276  // Search for the reference point (theta_*, phi_*) [notation of
277  // Bonazzola, Gourgoulhon & Marck PRD 58, 104020 (1998)]
278  // at the surface of the star
279  // ------------------------------------------------------------
280  double alpha_r2 = 0. ;
281 
282  for (int k=0; k<mg->get_np(l_b); k++) {
283  for (int j=0; j<mg->get_nt(l_b); j++) {
284 
285  double lapconf_auto_b =
286  lapconf_auto.val_grid_point(l_b,k,j,i_b) - 0.5 ;
287  double lapconf_comp_b =
288  lapconf_comp.val_grid_point(l_b,k,j,i_b) ;
289 
290  double confo_b = confo_tot.val_grid_point(l_b,k,j,i_b) ;
291 
292  double gam_b = gam.val_grid_point(l_b,k,j,i_b) ;
293  double gam0_b = gam0.val_grid_point(l_b,k,j,i_b) ;
294 
295  double aaa = (gam0_c*gam_b*hhh_b*confo_c)
296  / (gam0_b*gam_c*hhh_c*confo_b) ;
297 
298  // See Eq (100) from Gourgoulhon et al. (2001)
299  double alpha_r2_jk = (aaa * lapconf_comp_b - lapconf_comp_c
300  + 0.5 * (aaa - 1.))
301  / (lapconf_auto_c - aaa * lapconf_auto_b ) ;
302 
303  if (alpha_r2_jk > alpha_r2) {
304  alpha_r2 = alpha_r2_jk ;
305  k_b = k ;
306  j_b = j ;
307  }
308  }
309  }
310 
311  alpha_r = sqrt(alpha_r2) ;
312 
313  cout << "k_b, j_b, alpha_r: " << k_b << " " << j_b << " "
314  << alpha_r << endl ;
315 
316  // New value of lapconf_auto
317  // -------------------------
318 
319  lapconf_auto = alpha_r2 * (lapconf_auto - 0.5) + 0.5 ;
320  Scalar lapconf_tot_tmp = lapconf_auto + lapconf_comp ;
321  lapconf_tot_tmp.std_spectral_base() ;
322 
323  /*
324  confo_auto = alpha_r2 * (confo_auto - 0.5) + 0.5 ;
325  Scalar confo_tot_tmp = confo_auto + confo_comp ;
326  confo_tot_tmp.std_spectral_base() ;
327  */
328  //------------------------------------------------------------
329  // Change the values of the inner points of the second domain
330  // by those of the outer points of the first domain
331  //------------------------------------------------------------
332 
334 
335  //--------------------------------------------
336  // First integral --> enthalpy in all space
337  // See Eq (98) from Gourgoulhon et al. (2001)
338  //--------------------------------------------
339 
340  double log_lapconf_c = log(lapconf_tot_tmp.val_grid_point(0,0,0,0)) ;
341  double log_confo_c = log(confo_tot.val_grid_point(0,0,0,0)) ;
342  double loggam_c = loggam.val_grid_point(0,0,0,0) ;
343  double pot_centri_c = pot_centri.val_grid_point(0,0,0,0) ;
344 
345  ent = (ent_c + log_lapconf_c - log_confo_c + loggam_c + pot_centri_c)
346  - log(lapconf_tot_tmp) + log(confo_tot) - loggam - pot_centri ;
348 
349 
350  //----------------------------------------------------------
351  // Change the enthalpy field to be set its maximum position
352  // at the coordinate center
353  //----------------------------------------------------------
354 
355  double dentdx = ent.dsdx().val_grid_point(0,0,0,0) ;
356  double dentdy = ent.dsdy().val_grid_point(0,0,0,0) ;
357 
358  cout << "dH/dx|_center = " << dentdx << endl ;
359  cout << "dH/dy|_center = " << dentdy << endl ;
360 
361  double dec_fact_x = 1. ;
362  double dec_fact_y = 1. ;
363 
364  Scalar func_in(mp) ;
365  func_in = 1. - dec_fact_x * (dentdx/ent_c) * mp.x
366  - dec_fact_y * (dentdy/ent_c) * mp.y ;
367 
368  func_in.annule(nzet, nz-1) ;
369  func_in.std_spectral_base() ;
370 
371  Scalar func_ex(mp) ;
372  func_ex = 1. ;
373  func_ex.annule(0, nzet-1) ;
374  func_ex.std_spectral_base() ;
375 
376  // New enthalpy field
377  // ------------------
378  ent = ent * (func_in + func_ex) ;
379 
380  (ent.set_spectral_va()).smooth(nzet, ent.set_spectral_va()) ;
381 
382  double dentdx_new = ent.dsdx().val_grid_point(0,0,0,0) ;
383  double dentdy_new = ent.dsdy().val_grid_point(0,0,0,0) ;
384  cout << "dH/dx|_new = " << dentdx_new << endl ;
385  cout << "dH/dy|_new = " << dentdy_new << endl ;
386 
387  //-----------------------------------------------------
388  // Adaptation of the mapping to the new enthalpy field
389  //-----------------------------------------------------
390 
391  double dent_eq = ent.dsdr().val_point(ray_eq_pi(),M_PI/2.,M_PI) ;
392  double dent_pole = ent.dsdr().val_point(ray_pole(),0.,0.) ;
393  double rap_dent = fabs( dent_eq / dent_pole ) ;
394  cout << "| dH/dr_eq / dH/dr_pole | = " << rap_dent << endl ;
395  diff_dHdr = rap_dent ;
396 
397  if ( rap_dent < thres_adapt ) {
398  adapt_flag = 0 ; // No adaptation of the mapping
399  cout << "******* FROZEN MAPPING *********" << endl ;
400  }
401  else {
402  adapt_flag = 1 ; // The adaptation of the mapping is to be
403  // performed
404  }
405 
406  ent_limit.set_etat_qcq() ;
407  for (int l=0; l<nzet; l++) { // loop on domains inside the star
408  ent_limit.set(l) = ent.val_grid_point(l, k_b, j_b, i_b) ;
409  }
410  ent_limit.set(nzet-1) = ent_b ;
411 
412  Map_et mp_prev = mp_et ;
413 
414  Cmp ent_cmp(ent) ;
415  mp.adapt(ent_cmp, par_adapt) ;
416  ent = ent_cmp ;
417 
418  // Readjustment of the external boundary of domain l=nzet
419  // to keep a fixed ratio with respect to star's surface
420 
421  double rr_in_1 = mp.val_r(1, -1., M_PI/2., 0.) ;
422 
423  // Resize of the outer boundary of the shell including the BH
424  double rr_out_nm2 = mp.val_r(nz-2, 1., M_PI/2., 0.) ;
425  mp.resize(nz-2, rr_in_1/rr_out_nm2 * fact_resize(1)) ;
426 
427  // Resize of the inner boundary of the shell including the BH
428  double rr_out_nm3 = mp.val_r(nz-3, 1., M_PI/2., 0.) ;
429  mp.resize(nz-3, rr_in_1/rr_out_nm3 * fact_resize(0)) ;
430 
431  // if (mer % 2 == 0) {
432 
433  if (nz > 4) {
434 
435  // Resize of the domain 1
436  double rr_out_1 = mp.val_r(1, 1., M_PI/2., 0.) ;
437  mp.resize(1, rr_in_1/rr_out_1 * resize_ns) ;
438 
439  if (nz > 5) {
440 
441  // Resize of the domain from 2 to N-4
442  double rr_out_nm3_new = mp.val_r(nz-3, 1., M_PI/2., 0.) ;
443 
444  for (int i=1; i<nz-4; i++) {
445 
446  double rr_out_i = mp.val_r(i, 1., M_PI/2., 0.) ;
447 
448  double rr_mid = rr_out_i
449  + (rr_out_nm3_new - rr_out_i) / double(nz - 3 - i) ;
450 
451  double rr_2timesi = 2. * rr_out_i ;
452 
453  if (rr_2timesi < rr_mid) {
454 
455  double rr_out_ip1 = mp.val_r(i+1, 1., M_PI/2., 0.) ;
456  mp.resize(i+1, rr_2timesi / rr_out_ip1) ;
457 
458  }
459  else {
460 
461  double rr_out_ip1 = mp.val_r(i+1, 1., M_PI/2., 0.) ;
462  mp.resize(i+1, rr_mid / rr_out_ip1) ;
463 
464  } // End of else
465 
466  } // End of i loop
467 
468  } // End of (nz > 5) loop
469 
470  } // End of (nz > 4) loop
471 
472  // } // End of (mer % 2) loop
473 
474  //----------------------------------------------------
475  // Computation of the enthalpy at the new grid points
476  //----------------------------------------------------
477 
478  mp_prev.homothetie(alpha_r) ;
479 
480  Cmp ent_cmp2 (ent) ;
481  mp.reevaluate(&mp_prev, nzet+1, ent_cmp2) ;
482  ent = ent_cmp2 ;
483 
484  double ent_s_max = -1 ;
485  int k_s_max = -1 ;
486  int j_s_max = -1 ;
487 
488  for (int k=0; k<mg->get_np(l_b); k++) {
489  for (int j=0; j<mg->get_nt(l_b); j++) {
490  double xx = fabs( ent.val_grid_point(l_b, k, j, i_b) ) ;
491  if (xx > ent_s_max) {
492  ent_s_max = xx ;
493  k_s_max = k ;
494  j_s_max = j ;
495  }
496  }
497  }
498  cout << "Max. abs(enthalpy) at the boundary between domains nzet-1"
499  << " and nzet : " << endl ;
500  cout << " " << ent_s_max << " reached for k = " << k_s_max
501  << " and j = " << j_s_max << endl ;
502 
503  //-------------------
504  // Equation of state
505  //-------------------
506 
507  equation_of_state() ; // computes new values for nbar (n), ener (e)
508  // and press (p) from the new ent (H)
509 
510  //----------------------------------------------------------
511  // Matter source terms in the gravitational field equations
512  //----------------------------------------------------------
513 
514  hydro_euler_bhns(kerrschild, mass_bh, sepa) ;
515  // computes new values for ener_euler (E),
516  // s_euler (S) and u_euler (U^i)
517 
518 
519  //-------------------------------------------------
520  // Computation of the minimum of the indicator chi
521  //-------------------------------------------------
522  double azimu_min = phi_min() ;
523  double rad_chi_min = radius_p(azimu_min) ;
524  double chi_min = chi_rp(rad_chi_min, azimu_min) ;
525 
526  cout << "| dH/dr_eq / dH/dr_pole | (minimum) = " << chi_min << endl ;
527  cout << " phi = " << azimu_min / M_PI << " [M_PI]" << endl ;
528  cout << " radius = " << rad_chi_min / km << " [km]" << endl ;
529 
530  diff_dHdr_min = chi_min ;
531  diff_phi_min = azimu_min ;
532  diff_radius = rad_chi_min ;
533 
534  //-----------------------------------
535  // Poisson equation for lapconf_auto
536  //-----------------------------------
537 
538  // Source
539  //--------
540 
541  Scalar sou_lap1(mp) ; // dzpuis = 0
542  sou_lap1 = qpig * lapconf_tot_tmp * pow(confo_tot,4.)
543  * (0.5*ener_euler + s_euler) ;
544 
545  sou_lap1.std_spectral_base() ;
546  sou_lap1.annule(nzet,nz-1) ;
547  sou_lap1.inc_dzpuis(4) ; // dzpuis : 0 -> 4
548 
549  Scalar sou_lap2(mp) ; // dzpuis = 4
550  sou_lap2 = 0.875 * (lapconf_auto+0.5) * taij_quad_auto
551  / pow(confo_auto+0.5,8.) ;
552  sou_lap2.std_spectral_base() ;
553 
554  source_lapconf = sou_lap1 + sou_lap2 ;
555 
556  source_lapconf.std_spectral_base() ;
557  // source_lapse.annule(nzet,nz-1) ;
558 
559  if (filter_r != 0) {
560  if (source_lapconf.get_etat() != ETATZERO) {
561  source_lapconf.filtre(filter_r) ;
562  // source_lapse.filtre_r(filter_r,0) ;
563  }
564  }
565 
566  assert(source_lapconf.get_dzpuis() == 4) ;
567 
568  // Resolution of the Poisson equation (Outer BC : lapconf_m1 -> 0)
569  // ----------------------------------
570 
571  lapconf_m1.set_etat_qcq() ;
572  lapconf_m1 = lapconf_auto - 0.5 ;
573  source_lapconf.poisson(par_lapconf, lapconf_m1) ;
574  ssjm1_lapconf = ssjm1lapconf ;
575 
576  // Check: has the Poisson equation been correctly solved ?
577  // -------------------------------------------------------
578 
579  Tbl tdiff_lapconf = diffrel(lapconf_m1.laplacian(), source_lapconf) ;
580  cout <<
581  "Relative error in the resolution of the equation for lapconf_auto : "
582  << endl ;
583  for (int l=0; l<nz; l++) {
584  cout << tdiff_lapconf(l) << " " ;
585  }
586  cout << endl ;
587  diff_lapconf = max(abs(tdiff_lapconf)) ;
588 
589  // Re-construction of the lapconf function
590  // ---------------------------------------
591  lapconf_auto = lapconf_m1 + 0.5 ;
592  // lapconf_tot = lapconf_auto + lapconf_comp
593  // lapconf_auto, _comp -> 0.5 (r -> inf)
594  // lapconf_tot -> 1 (r -> inf)
595 
596  //---------------------------------
597  // Poisson equation for confo_auto
598  //---------------------------------
599 
600  // Source
601  //--------
602 
603  Scalar sou_con1(mp) ; // dzpuis = 0
604  sou_con1 = - 0.5 * qpig * pow(confo_tot,5.) * ener_euler ;
605  sou_con1.std_spectral_base() ;
606  sou_con1.annule(nzet,nz-1) ;
607  sou_con1.inc_dzpuis(4) ; // dzpuis : 0 -> 4
608 
609  Scalar sou_con2(mp) ; // dzpuis = 4
610  sou_con2 = - 0.125 * taij_quad_auto / pow(confo_auto+0.5,7.) ;
611  sou_con2.std_spectral_base() ;
612 
613  source_confo = sou_con1 + sou_con2 ;
614 
615  source_confo.std_spectral_base() ;
616  // source_confo.annule(nzet,nz-1) ;
617 
618  if (filter_r != 0) {
619  if (source_confo.get_etat() != ETATZERO) {
620  source_confo.filtre(filter_r) ;
621  // source_confo.filtre_r(filter_r,0) ;
622  }
623  }
624 
625  assert(source_confo.get_dzpuis() == 4) ;
626 
627  // Resolution of the Poisson equation (Outer BC : confo_m1 -> 0)
628  // ----------------------------------
629 
630  confo_m1.set_etat_qcq() ;
631  confo_m1 = confo_auto - 0.5 ;
632  source_confo.poisson(par_confo, confo_m1) ;
633  ssjm1_confo = ssjm1confo ;
634 
635  // Check: has the Poisson equation been correctly solved ?
636  // -------------------------------------------------------
637 
638  Tbl tdiff_confo = diffrel(confo_m1.laplacian(), source_confo) ;
639  cout <<
640  "Relative error in the resolution of the equation for confo_auto : "
641  << endl ;
642  for (int l=0; l<nz; l++) {
643  cout << tdiff_confo(l) << " " ;
644  }
645  cout << endl ;
646  diff_confo = max(abs(tdiff_confo)) ;
647 
648  // Re-construction of the conformal factor
649  // ---------------------------------------
650  confo_auto = confo_m1 + 0.5 ; // confo_tot = confo_auto + confo_comp
651  // confo_auto, _comp -> 0.5 (r -> inf)
652  // confo_tot -> 1 (r -> inf)
653 
654  //----------------------------------------
655  // Vector Poisson equation for shift_auto
656  //----------------------------------------
657 
658  // Source
659  // ------
660 
661  Vector sou_shif1(mp, CON, mp.get_bvect_cart()) ; // dzpuis = 0
662  sou_shif1.set_etat_qcq() ;
663 
664  for (int i=1; i<=3; i++) {
665  sou_shif1.set(i) = 4.*qpig * lapconf_tot_tmp
666  * pow(confo_tot, 3.)
667  * (ener_euler + press) * u_euler(i) ;
668  }
669 
670  sou_shif1.std_spectral_base() ;
671  sou_shif1.annule(nzet, nz-1) ;
672 
673  for (int i=1; i<=3; i++) {
674  (sou_shif1.set(i)).inc_dzpuis(4) ; // dzpuis: 0 -> 4
675  }
676 
677  Vector sou_shif2(mp, CON, mp.get_bvect_cart()) ; // dzpuis = 4
678  sou_shif2.set_etat_qcq() ;
679  for (int i=1; i<=3; i++) {
680  sou_shif2.set(i) = 2. *
681  (taij_auto(i,1)*(d_lapconf_auto(1)
682  -7.*(lapconf_auto+0.5)*d_confo_auto(1)
683  /(confo_auto+0.5))
684  +taij_auto(i,2)*(d_lapconf_auto(2)
685  -7.*(lapconf_auto+0.5)*d_confo_auto(2)
686  /(confo_auto+0.5))
687  +taij_auto(i,3)*(d_lapconf_auto(3)
688  -7.*(lapconf_auto+0.5)*d_confo_auto(3)
689  /(confo_auto+0.5))
690  ) / pow(confo_auto+0.5,7.) ;
691  }
692  sou_shif2.std_spectral_base() ;
693 
694  source_shift = sou_shif1 + sou_shif2 ;
695 
696  source_shift.std_spectral_base() ;
697  // source_shift.annule(nzet, nz-1) ;
698 
699  // Resolution of the Poisson equation
700  // ----------------------------------
701 
702  // Filter for the source of shift vector
703 
704  if (filter_r_s != 0) {
705  for (int i=1; i<=3; i++) {
706  if (source_shift(i).get_etat() != ETATZERO) {
707  source_shift.set(i).filtre(filter_r_s) ;
708  // source_shift.set(i).filtre_r(filter_r_s, 0) ;
709  }
710  }
711  }
712 
713  if (filter_p_s != 0) {
714  for (int i=1; i<=3; i++) {
715  if (source_shift(i).get_etat() != ETATZERO) {
716  (source_shift.set(i)).filtre_phi(filter_p_s, nz-1) ;
717  // (source_shift.set(i)).filtre_phi(filter_p_s, 0) ;
718  }
719  }
720  }
721 
722  for (int i=1; i<=3; i++) {
723  if(source_shift(i).dz_nonzero()) {
724  assert( source_shift(i).get_dzpuis() == 4 ) ;
725  }
726  else {
727  (source_shift.set(i)).set_dzpuis(4) ;
728  }
729  }
730 
731  double lambda = double(1) / double(3) ;
732 
733  Tenseur source_p(mp, 1, CON, mp.get_bvect_cart() ) ;
734  source_p.set_etat_qcq() ;
735  for (int i=0; i<3; i++) {
736  source_p.set(i) = Cmp(source_shift(i+1)) ;
737  }
738 
739  Tenseur vect_auxi(mp, 1, CON, mp.get_bvect_cart()) ;
740  vect_auxi.set_etat_qcq() ;
741  for (int i=0; i<3 ;i++) {
742  vect_auxi.set(i) = 0. ;
743  }
744  Tenseur scal_auxi(mp) ;
745  scal_auxi.set_etat_qcq() ;
746  scal_auxi.set().annule_hard() ;
747  scal_auxi.set_std_base() ;
748 
749  Tenseur resu_p(mp, 1, CON, mp.get_bvect_cart() ) ;
750  resu_p.set_etat_qcq() ;
751 
752  source_p.poisson_vect(lambda, par_shift2, resu_p, vect_auxi,
753  scal_auxi) ;
754 
755  for (int i=1; i<=3; i++)
756  shift_auto.set(i) = resu_p(i-1) ;
757 
758  ssjm1_khi = ssjm1khi ;
759 
760  for (int i=0; i<3; i++) {
761  ssjm1_wshift.set(i+1) = ssjm1wshift(i) ;
762  }
763 
764  // Check: has the equation for shift_auto been correctly solved ?
765  // --------------------------------------------------------------
766 
768  + lambda * shift_auto.divergence(flat).derive_con(flat) ;
769 
770  source_shift.dec_dzpuis() ;
771 
772  Tbl tdiff_shift_x = diffrel(lap_shift(1), source_shift(1)) ;
773  Tbl tdiff_shift_y = diffrel(lap_shift(2), source_shift(2)) ;
774  Tbl tdiff_shift_z = diffrel(lap_shift(3), source_shift(3)) ;
775 
776  cout <<
777  "Relative error in the resolution of the equation for shift_auto : "
778  << endl ;
779  cout << "x component : " ;
780  for (int l=0; l<nz; l++) {
781  cout << tdiff_shift_x(l) << " " ;
782  }
783  cout << endl ;
784  cout << "y component : " ;
785  for (int l=0; l<nz; l++) {
786  cout << tdiff_shift_y(l) << " " ;
787  }
788  cout << endl ;
789  cout << "z component : " ;
790  for (int l=0; l<nz; l++) {
791  cout << tdiff_shift_z(l) << " " ;
792  }
793  cout << endl ;
794 
795  diff_shift_x = max(abs(tdiff_shift_x)) ;
796  diff_shift_y = max(abs(tdiff_shift_y)) ;
797  diff_shift_z = max(abs(tdiff_shift_z)) ;
798 
799 
800  //-----------------------------
801  // Relative change in enthalpy
802  //-----------------------------
803 
804  Tbl diff_ent_tbl = diffrel( ent, ent_jm1 ) ;
805  diff_ent = diff_ent_tbl(0) ;
806  for (int l=0; l<nzet; l++) {
807  diff_ent += diff_ent_tbl(l) ;
808  }
809  diff_ent /= nzet ;
810 
811  ent_jm1 = ent ;
812 
813  /*
814  des_profile( lapconf_auto, 0., 10.,
815  M_PI/2., M_PI, "Self lapconf function of NS",
816  "Lapconf (theta=pi/2, phi=0)" ) ;
817 
818  des_profile( lapconf_tot, 0., 10.,
819  M_PI/2., M_PI, "Total lapconf function seen by NS",
820  "Lapconf (theta=pi/2, phi=0)" ) ;
821 
822  des_profile( confo_auto, 0., 10.,
823  M_PI/2., M_PI, "Self conformal factor of NS",
824  "Confo (theta=pi/2, phi=0)" ) ;
825 
826  des_profile( confo_tot, 0., 10.,
827  M_PI/2., M_PI, "Total conformal factor seen by NS",
828  "Confo (theta=pi/2, phi=0)" ) ;
829 
830  des_coupe_vect_z( shift_auto, 0., -3., 0.5, 3,
831  "Self shift vector of NS") ;
832 
833  des_coupe_vect_z( shift_tot, 0., -3., 0.5, 3,
834  "Total shift vector seen by NS") ;
835  */
836  } // End of main loop
837 
838  //=========================================================
839  // End of iteration
840  //=========================================================
841 
842 
843 }
844 }
Vector d_lapconf_auto
Derivative of the lapconf function generated by the star .
Definition: star_bhns.h:130
Cmp log(const Cmp &)
Neperian logarithm.
Definition: cmp_math.C:299
virtual void set_etat_qcq()
Sets the logical state of all components to ETATQCQ (ordinary state).
Definition: tensor.C:490
void hydro_euler_bhns(bool kerrschild, const double &mass_bh, const double &sepa)
Computes the hydrodynamical quantities relative to the Eulerian observer from those in the fluid fram...
void add_tenseur_mod(Tenseur &ti, int position=0)
Adds the address of a new modifiable Tenseur to the list.
Definition: param.C:1145
Component of a tensorial field *** DEPRECATED : use class Scalar instead ***.
Definition: cmp.h:446
Cmp exp(const Cmp &)
Exponential.
Definition: cmp_math.C:273
Radial mapping of rather general form.
Definition: map.h:2783
void add_int(const int &n, int position=0)
Adds the address of a new int to the list.
Definition: param.C:249
Map & mp
Mapping associated with the star.
Definition: star.h:180
Scalar ssjm1_khi
Effective source at the previous step for the resolution of the Poisson equation for the scalar by m...
Definition: star_bhns.h:210
int get_np(int l) const
Returns the number of points in the azimuthal direction ( ) in domain no. l.
Definition: grilles.h:479
Cmp sqrt(const Cmp &)
Square root.
Definition: cmp_math.C:223
virtual void annule(int l_min, int l_max)
Sets the Scalar to zero in several domains.
Definition: scalar.C:397
void set_std_base()
Set the standard spectal basis of decomposition for each component.
Definition: tenseur.C:1186
Lorene prototypes.
Definition: app_hor.h:67
Standard units of space, time and mass.
const Mg3d * get_mg() const
Gives the Mg3d on which the mapping is defined.
Definition: map.h:783
const Scalar & laplacian(int ced_mult_r=4) const
Returns the Laplacian of *this.
Definition: scalar_deriv.C:436
double & set(int i)
Read/write of a particular element (index i) (1D case)
Definition: tbl.h:301
Tensor field of valence 0 (or component of a tensorial field).
Definition: scalar.h:393
Scalar poisson() const
Solves the scalar Poisson equation with *this as a source.
Definition: scalar_pde.C:139
virtual void adapt(const Cmp &ent, const Param &par, int nbr=0)=0
Adaptation of the mapping to a given scalar field.
Scalar loggam
Logarithm of the Lorentz factor between the fluid and the co-orbiting observer.
Definition: star_bhns.h:93
const Scalar & dsdx() const
Returns of *this , where .
Definition: scalar_deriv.C:266
virtual void std_spectral_base()
Sets the spectral bases of the Valeur va to the standard ones for a scalar field. ...
Definition: scalar.C:790
void annule_hard()
Sets the Cmp to zero in a hard way.
Definition: cmp.C:341
int get_etat() const
Returns the logical state ETATNONDEF (undefined), ETATZERO (null) or ETATQCQ (ordinary).
Definition: scalar.h:560
Scalar ent
Log-enthalpy.
Definition: star.h:190
Vector shift_auto
Shift vector generated by the star.
Definition: star_bhns.h:138
Scalar s_euler
Trace of the stress scalar in the Eulerian frame.
Definition: star.h:201
virtual void set_etat_qcq()
Sets the logical state to ETATQCQ (ordinary state).
Definition: scalar.C:359
const Vector & derive_con(const Metric &gam) const
Returns the "contravariant" derivative of *this with respect to some metric , by raising the index of...
Definition: scalar_deriv.C:402
Tensor field of valence 1.
Definition: vector.h:188
void smooth(int nzet, Valeur &uuva) const
Changes the function *this as a smooth one when there exists a discontinuity between the nucleus and ...
Definition: valeur_smooth.C:80
Tbl diffrel(const Cmp &a, const Cmp &b)
Relative difference between two Cmp (norme version).
Definition: cmp_math.C:507
Scalar gam
Lorentz factor between the fluid and the co-orbiting observer.
Definition: star_bhns.h:102
double val_grid_point(int l, int k, int j, int i) const
Returns the value of the field at a specified grid point.
Definition: scalar.h:643
virtual void std_spectral_base()
Sets the standard spectal bases of decomposition for each component.
Definition: vector.C:322
virtual void dec_dzpuis(int dec=1)
Decreases by dec units the value of dzpuis and changes accordingly the values in the compactified ext...
Definition: tensor.C:817
void set_etat_qcq()
Sets the logical state to ETATQCQ (ordinary state).
Definition: tbl.C:364
int nzet
Number of domains of *mp occupied by the star.
Definition: star.h:183
Metric_flat flat
Flat metric defined on the mapping (Spherical components with respect to the mapping of the star )...
Definition: star_bhns.h:192
Scalar confo_tot
Total conformal factor.
Definition: star_bhns.h:163
virtual double val_r(int l, double xi, double theta, double pphi) const =0
Returns the value of the radial coordinate r for a given in a given domain.
Cmp & set()
Read/write for a scalar (see also operator=(const Cmp&) ).
Definition: tenseur.C:840
virtual void inc_dzpuis(int inc=1)
Increases by inc units the value of dzpuis and changes accordingly the values of the Scalar in the co...
Scalar press
Fluid pressure.
Definition: star.h:194
const Scalar & dsdy() const
Returns of *this , where .
Definition: scalar_deriv.C:297
int get_dzpuis() const
Returns dzpuis.
Definition: scalar.h:563
Parameter storage.
Definition: param.h:125
void add_tbl(const Tbl &ti, int position=0)
Adds the address of a new Tbl to the list.
Definition: param.C:525
double radius_p(double phi)
Radius of the star to the direction of and .
Definition: star_bhns_chi.C:77
int get_nzone() const
Returns the number of domains.
Definition: grilles.h:465
virtual void homothetie(double lambda)
Sets a new radial scale.
Definition: map_et.C:928
Tbl max(const Cmp &)
Maximum values of a Cmp in each domain.
Definition: cmp_math.C:438
const Scalar & divergence(const Metric &) const
The divergence of this with respect to a Metric .
Definition: vector.C:387
Scalar lapconf_comp
Lapconf function generated by the companion black hole.
Definition: star_bhns.h:116
Vector u_euler
Fluid 3-velocity with respect to the Eulerian observer.
Definition: star.h:207
double ray_eq_pi() const
Coordinate radius at , [r_unit].
Definition: star_global.C:189
Scalar taij_quad_auto
Part of the scalar generated by .
Definition: star_bhns.h:187
Cmp pow(const Cmp &, int)
Power .
Definition: cmp_math.C:351
void set_etat_qcq()
Sets the logical state to ETATQCQ (ordinary state).
Definition: cmp.C:307
void filtre(int n)
Sets the n lasts coefficients in r to 0 in the external domain.
Definition: scalar_manip.C:157
Scalar gam0
Lorentz factor between the co-orbiting observer and the Eulerian one.
Definition: star_bhns.h:107
Vector ssjm1_wshift
Effective source at the previous step for the resolution of the vector Poisson equation for by means...
Definition: star_bhns.h:220
virtual void resize(int l, double lambda)=0
Rescales the outer boundary of one domain.
Scalar pot_centri
Centrifugal potential.
Definition: star_bhns.h:110
const Tensor & divergence(const Metric &gam) const
Computes the divergence of this with respect to some metric .
Definition: tensor.C:1064
double val_point(double r, double theta, double phi) const
Computes the value of the field at an arbitrary point , by means of the spectral expansion.
Definition: scalar.C:896
double phi_min()
Azimuthal angle when the indicator of the mass-shedding takes its minimum chi_min.
Definition: star_bhns_chi.C:86
double ray_pole() const
Coordinate radius at [r_unit].
Definition: star_global.C:281
double chi_rp(double radius, double phi)
Sensitive indicator of the mass-shedding to the direction of , , .
Definition: star_bhns_chi.C:64
Scalar lapconf_auto
Lapconf function generated by the star.
Definition: star_bhns.h:113
int get_nr(int l) const
Returns the number of points in the radial direction ( ) in domain no. l.
Definition: grilles.h:469
const Tensor & derive_con(const Metric &gam) const
Returns the "contravariant" derivative of this with respect to some metric , by raising the last inde...
Definition: tensor.C:1023
bool irrotational
true for an irrotational star, false for a corotating one
Definition: star_bhns.h:72
Multi-domain grid.
Definition: grilles.h:279
const Base_vect_cart & get_bvect_cart() const
Returns the Cartesian basis associated with the coordinates (x,y,z) of the mapping, i.e.
Definition: map.h:809
Vector d_confo_auto
Derivative of the conformal factor generated by the star .
Definition: star_bhns.h:168
Scalar confo_auto
Conformal factor generated by the star.
Definition: star_bhns.h:157
Coord y
y coordinate centered on the grid
Definition: map.h:745
Cmp abs(const Cmp &)
Absolute value.
Definition: cmp_math.C:413
virtual void reevaluate(const Map *mp_prev, int nzet, Cmp &uu) const =0
Recomputes the values of a Cmp at the collocation points after a change in the mapping.
void add_double(const double &x, int position=0)
Adds the the address of a new double to the list.
Definition: param.C:318
const Scalar & dsdr() const
Returns of *this .
Definition: scalar_deriv.C:113
Sym_tensor taij_auto
Part of the extrinsic curvature tensor generated by shift_auto , lapse_auto , and confo_auto ...
Definition: star_bhns.h:182
Coord x
x coordinate centered on the grid
Definition: map.h:744
void equilibrium_bhns(double ent_c, const double &mass_bh, const double &sepa, bool kerrschild, int mer, int mermax_ns, int mermax_potvit, int mermax_poisson, int filter_r, int filter_r_s, int filter_p_s, double relax_poisson, double relax_potvit, double thres_adapt, double resize_ns, const Tbl &fact_resize, Tbl &diff)
Computes an equilibrium configuration.
Scalar ssjm1_lapconf
Effective source at the previous step for the resolution of the Poisson equation for lapconf_auto ...
Definition: star_bhns.h:197
Basic array class.
Definition: tbl.h:164
int get_nt(int l) const
Returns the number of points in the co-latitude direction ( ) in domain no. l.
Definition: grilles.h:474
Valeur & set_spectral_va()
Returns va (read/write version)
Definition: scalar.h:610
Scalar & set(int)
Read/write access to a component.
Definition: vector.C:302
void set_etat_qcq()
Sets the logical state to ETATQCQ (ordinary state).
Definition: tenseur.C:652
void add_cmp_mod(Cmp &ti, int position=0)
Adds the address of a new modifiable Cmp to the list.
Definition: param.C:1007
void equation_of_state()
Computes the proper baryon and energy density, as well as pressure from the enthalpy.
Definition: star.C:465
Scalar ssjm1_confo
Effective source at the previous step for the resolution of the Poisson equation for confo_auto ...
Definition: star_bhns.h:202
Scalar ener_euler
Total energy density in the Eulerian frame.
Definition: star.h:198
Tensor handling *** DEPRECATED : use class Tensor instead ***.
Definition: tenseur.h:304
void add_int_mod(int &n, int position=0)
Adds the address of a new modifiable int to the list.
Definition: param.C:388
double velo_pot_bhns(const double &mass_bh, const double &sepa, bool kerrschild, int mermax, double precis, double relax)
Computes the non-translational part of the velocity scalar potential by solving the continuity equat...