LORENE
et_bfrot_equilibre.C
1 /*
2  * Method of class Et_rot_bifluid to compute a static spherical configuration.
3  *
4  * (see file etoile.h for documentation).
5  *
6  */
7 
8 /*
9  * Copyright (c) 2001 Jerome Novak
10  *
11  * This file is part of LORENE.
12  *
13  * LORENE is free software; you can redistribute it and/or modify
14  * it under the terms of the GNU General Public License as published by
15  * the Free Software Foundation; either version 2 of the License, or
16  * (at your option) any later version.
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 /*
33  * $Id: et_bfrot_equilibre.C,v 1.22 2017/10/06 12:36:34 a_sourie Exp $
34  * $Log: et_bfrot_equilibre.C,v $
35  * Revision 1.22 2017/10/06 12:36:34 a_sourie
36  * Cleaning of tabulated 2-fluid EoS class + superfluid rotating star model.
37  *
38  * Revision 1.21 2016/12/05 16:17:52 j_novak
39  * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
40  *
41  * Revision 1.20 2015/06/10 14:39:17 a_sourie
42  * New class Eos_bf_tabul for tabulated 2-fluid EoSs and associated functions for the computation of rotating stars with such EoSs.
43  *
44  * Revision 1.19 2014/10/13 08:52:54 j_novak
45  * Lorene classes and functions now belong to the namespace Lorene.
46  *
47  * Revision 1.18 2014/10/06 15:13:07 j_novak
48  * Modified #include directives to use c++ syntax.
49  *
50  * Revision 1.17 2006/03/13 10:02:27 j_novak
51  * Added things for triaxial perturbations.
52  *
53  * Revision 1.16 2004/09/01 10:56:05 r_prix
54  * added option of converging baryon-mass to equilibrium_bi()
55  *
56  * Revision 1.15 2004/08/30 09:54:20 r_prix
57  * experimental version of Kepler-limit finder for 2-fluid stars
58  *
59  * Revision 1.14 2004/03/25 10:29:03 j_novak
60  * All LORENE's units are now defined in the namespace Unites (in file unites.h).
61  *
62  * Revision 1.13 2003/12/11 12:43:35 r_prix
63  * activated adaptive grid for 2-fluid star (taken from Etoile_rot)
64  *
65  * Revision 1.12 2003/12/04 14:28:26 r_prix
66  * allow for the case of "slow-rot-style" EOS inversion, in which we need to adapt
67  * the inner domain to n_outer=0 instead of mu_outer=0 ...
68  * (this should only be used for comparison to analytic slow-rot solution!)
69  *
70  * Revision 1.11 2003/11/25 12:49:44 j_novak
71  * Modified headers to compile on IRIX. Changed Mapping to be Map_af (speed
72  * enhancement).
73  *
74  * Revision 1.10 2003/11/20 14:01:25 r_prix
75  * changed member names to better conform to Lorene coding standards:
76  * J_euler -> j_euler, EpS_euler -> enerps_euler, Delta_car -> delta_car
77  *
78  * Revision 1.9 2003/11/19 22:01:57 e_gourgoulhon
79  * -- Relaxation on logn and dzeta performed only if mer >= 10.
80  * -- err_grv2 is now evaluated also in the Newtonian case.
81  *
82  * Revision 1.8 2003/11/18 18:38:11 r_prix
83  * use of new member EpS_euler: matter sources in equilibrium() and global quantities
84  * no longer distinguish Newtonian/relativistic, as all terms should have the right limit...
85  *
86  * Revision 1.7 2003/11/17 13:49:43 r_prix
87  * - moved superluminal check into hydro_euler()
88  * - removed some warnings
89  *
90  * Revision 1.6 2003/11/13 12:14:35 r_prix
91  * *) removed all use of etoile-type specific u_euler, press
92  * and use 3+1 components of Tmunu instead
93  *
94  * Revision 1.5 2002/10/16 14:36:35 j_novak
95  * Reorganization of #include instructions of standard C++, in order to
96  * use experimental version 3 of gcc.
97  *
98  * Revision 1.4 2002/04/05 09:09:36 j_novak
99  * The inversion of the EOS for 2-fluids polytrope has been modified.
100  * Some errors in the determination of the surface were corrected.
101  *
102  * Revision 1.3 2002/01/16 15:03:28 j_novak
103  * *** empty log message ***
104  *
105  * Revision 1.2 2002/01/03 15:30:28 j_novak
106  * Some comments modified.
107  *
108  * Revision 1.1.1.1 2001/11/20 15:19:28 e_gourgoulhon
109  * LORENE
110  *
111  * Revision 1.1 2001/06/22 15:40:06 novak
112  * Initial revision
113  *
114  *
115  * $Header: /cvsroot/Lorene/C++/Source/Etoile/et_bfrot_equilibre.C,v 1.22 2017/10/06 12:36:34 a_sourie Exp $
116  *
117  */
118 
119 // Headers C
120 #include <cmath>
121 
122 // Headers Lorene
123 #include "et_rot_bifluid.h"
124 #include "param.h"
125 #include "unites.h"
126 
127 #include "graphique.h"
128 #include "utilitaires.h"
129 
130 namespace Lorene {
131 
132 //-------------------------------------------------------------------------
133 //-------------------------------------------------------------------------
134 
135 // Axial Equilibrium
136 
137 //-------------------------------------------------------------------------
138 //-------------------------------------------------------------------------
139 
141 (double ent_c, double ent2_c, double omega0, double omega20,
142  const Tbl& ent_limit, const Tbl& ent2_limit, const Itbl& icontrol,
143  const Tbl& control, Tbl& diff,
144  int mer_mass, double mbar1_wanted, double mbar2_wanted, double aexp_mass)
145 {
146 
147  // Fundamental constants and units
148  // -------------------------------
149  using namespace Unites ;
150 
151  // For the display
152  // ---------------
153  char display_bold[]="x[1m" ; display_bold[0] = 27 ;
154  char display_normal[] = "x[0m" ; display_normal[0] = 27 ;
155 
156  // Grid parameters
157  // ---------------
158 
159  const Mg3d* mg = mp.get_mg() ;
160  int nz = mg->get_nzone() ; // total number of domains
161 
162  // The following is required to initialize mp_prev as a Map_af
163  Map_et& mp_et = dynamic_cast<Map_et&>(mp) ; // reference
164 
165  // Index of the point at phi=0, theta=pi/2 at the surface of the star:
166  assert(mg->get_type_t() == SYM) ;
167  int l_b = nzet - 1 ;
168  int i_b = mg->get_nr(l_b) - 1 ;
169  int j_b = mg->get_nt(l_b) - 1 ;
170  int k_b = 0 ;
171 
172  // Value of the enthalpies defining the surface of each fluid
173  double ent1_b = ent_limit(nzet-1) ;
174  double ent2_b = ent2_limit(nzet-1) ;
175 
176  // This value is chosen so that the grid contain both fluids
177 // double ent_b = (ent1_b > ent2_b ? ent1_b : ent2_b) ;
178 
179  // Parameters to control the iteration
180  // -----------------------------------
181 
182  int mer_max = icontrol(0) ;
183  int mer_rot = icontrol(1) ;
184  int mer_change_omega = icontrol(2) ;
185  int mer_fix_omega = icontrol(3) ;
186  int mermax_poisson = icontrol(4) ;
187  int nzadapt = icontrol(5); // number of domains for adaptive grid
188  int kepler_fluid = icontrol(6); // fluid-index for kepler-limit (0=none,3=both)
189  int kepler_wait_steps = icontrol(7);
190  int mer_triax = icontrol(8) ;
191 
192  int niter ;
193 
194  // Protections:
195  if (mer_change_omega < mer_rot) {
196  cout << "Et_rot_bifluid::equilibrium: mer_change_omega < mer_rot !" << endl ;
197  cout << " mer_change_omega = " << mer_change_omega << endl ;
198  cout << " mer_rot = " << mer_rot << endl ;
199  abort() ;
200  }
201  if (mer_fix_omega < mer_change_omega) {
202  cout << "Et_rot_bifluid::equilibrium: mer_fix_omega < mer_change_omega !"
203  << endl ;
204  cout << " mer_fix_omega = " << mer_fix_omega << endl ;
205  cout << " mer_change_omega = " << mer_change_omega << endl ;
206  abort() ;
207  }
208 
209  double precis = control(0) ;
210  double omega_ini = control(1) ;
211  double omega2_ini = control(2) ;
212  double relax = control(3) ;
213  double relax_prev = double(1) - relax ;
214  double relax_poisson = control(4) ;
215  // some additional stuff for adaptive grid:
216  double thres_adapt = control(5) ;
217  double precis_adapt = control(6) ;
218  double kepler_factor = control(7);
219  if (kepler_factor <= 1.0)
220  {
221  cout << "ERROR: Kepler factor has to be greater than 1!!\n";
222  abort();
223  }
224  double ampli_triax = control(8) ;
225 
226  // Error indicators
227  // ----------------
228 
229  diff.set_etat_qcq() ;
230  double diff_ent ;
231  double& diff_ent1 = diff.set(0) ;
232  double& diff_ent2 = diff.set(1) ;
233  double& diff_nuf = diff.set(2) ;
234  double& diff_nuq = diff.set(3) ;
235  // double& diff_dzeta = diff.set(4) ;
236  // double& diff_ggg = diff.set(5) ;
237  double& diff_shift_x = diff.set(6) ;
238  double& diff_shift_y = diff.set(7) ;
239  double& vit_triax = diff.set(8) ;
240 
241  // Parameters for the function Map_et::adapt
242  // -----------------------------------------
243 
244  Param par_adapt ;
245  int nitermax = 100 ;
246  int adapt_flag = 1 ; // 1 = performs the full computation,
247  // 0 = performs only the rescaling by
248  // the factor alpha_r
249  int nz_search = nzet + 1 ; // Number of domains for searching the enthalpy
250  // isosurfaces
251  double alpha_r ;
252  double reg_map = 1. ; // 1 = regular mapping, 0 = contracting mapping
253 
254  par_adapt.add_int(nitermax, 0) ; // maximum number of iterations to
255  // locate zeros by the secant method
256  par_adapt.add_int(nzadapt, 1) ; // number of domains where the adjustment
257  // to the isosurfaces of ent is to be
258  // performed
259  par_adapt.add_int(nz_search, 2) ; // number of domains to search for
260  // the enthalpy isosurface
261  par_adapt.add_int(adapt_flag, 3) ; // 1 = performs the full computation,
262  // 0 = performs only the rescaling by
263  // the factor alpha_r
264  par_adapt.add_int(j_b, 4) ; // theta index of the collocation point
265  // (theta_*, phi_*)
266  par_adapt.add_int(k_b, 5) ; // theta index of the collocation point
267  // (theta_*, phi_*)
268 
269  par_adapt.add_int_mod(niter, 0) ; // number of iterations actually used in
270  // the secant method
271 
272  par_adapt.add_double(precis_adapt, 0) ; // required absolute precision in
273  // the determination of zeros by
274  // the secant method
275  par_adapt.add_double(reg_map, 1) ; // 1. = regular mapping, 0 = contracting mapping
276 
277  par_adapt.add_double(alpha_r, 2) ; // factor by which all the radial
278  // distances will be multiplied
279 
280  par_adapt.add_tbl(ent_limit, 0) ; // array of values of the field ent
281  // to define the isosurfaces.
282 
283 
284  // Parameters for the function Map_et::poisson for nuf
285  // ----------------------------------------------------
286 
287  double precis_poisson = 1.e-16 ;
288 
289  Param par_poisson_nuf ;
290  par_poisson_nuf.add_int(mermax_poisson, 0) ; // maximum number of iterations
291  par_poisson_nuf.add_double(relax_poisson, 0) ; // relaxation parameter
292  par_poisson_nuf.add_double(precis_poisson, 1) ; // required precision
293  par_poisson_nuf.add_int_mod(niter, 0) ; // number of iterations actually used
294  par_poisson_nuf.add_cmp_mod( ssjm1_nuf ) ;
295 
296  Param par_poisson_nuq ;
297  par_poisson_nuq.add_int(mermax_poisson, 0) ; // maximum number of iterations
298  par_poisson_nuq.add_double(relax_poisson, 0) ; // relaxation parameter
299  par_poisson_nuq.add_double(precis_poisson, 1) ; // required precision
300  par_poisson_nuq.add_int_mod(niter, 0) ; // number of iterations actually used
301  par_poisson_nuq.add_cmp_mod( ssjm1_nuq ) ;
302 
303  Param par_poisson_tggg ;
304  par_poisson_tggg.add_int(mermax_poisson, 0) ; // maximum number of iterations
305  par_poisson_tggg.add_double(relax_poisson, 0) ; // relaxation parameter
306  par_poisson_tggg.add_double(precis_poisson, 1) ; // required precision
307  par_poisson_tggg.add_int_mod(niter, 0) ; // number of iterations actually used
308  par_poisson_tggg.add_cmp_mod( ssjm1_tggg ) ;
309  double lambda_tggg ;
310  par_poisson_tggg.add_double_mod( lambda_tggg ) ;
311 
312  Param par_poisson_dzeta ;
313  double lbda_grv2 ;
314  par_poisson_dzeta.add_double_mod( lbda_grv2 ) ;
315 
316  // Parameters for the function Tenseur::poisson_vect
317  // -------------------------------------------------
318 
319  Param par_poisson_vect ;
320 
321  par_poisson_vect.add_int(mermax_poisson, 0) ; // maximum number of iterations
322  par_poisson_vect.add_double(relax_poisson, 0) ; // relaxation parameter
323  par_poisson_vect.add_double(precis_poisson, 1) ; // required precision
324  par_poisson_vect.add_cmp_mod( ssjm1_khi ) ;
325  par_poisson_vect.add_tenseur_mod( ssjm1_wshift ) ;
326  par_poisson_vect.add_int_mod(niter, 0) ;
327 
328 
329  // Initializations
330  // ---------------
331 
332  // Initial angular velocities
333  omega = 0 ;
334  omega2 = 0 ;
335 
336  double accrois_omega = (omega0 - omega_ini) /
337  double(mer_fix_omega - mer_change_omega) ;
338  double accrois_omega2 = (omega20 - omega2_ini) /
339  double(mer_fix_omega - mer_change_omega) ;
340 
341 
342  update_metric() ; // update of the metric coefficients
343 
344  equation_of_state() ; // update of the densities, pressure, etc...
345 
346  hydro_euler() ; // update of the hydro quantities relative to the
347  // Eulerian observer
348 
349  // Quantities at the previous step :
350 
351  Map_et mp_prev = mp_et;
352  Tenseur ent_prev = ent ;
353  Tenseur ent2_prev = ent2 ;
354  Tenseur logn_prev = logn ;
355  Tenseur dzeta_prev = dzeta ;
356 
357  // Creation of uninitialized tensors:
358  Tenseur source_nuf(mp) ; // source term in the equation for nuf
359  Tenseur source_nuq(mp) ; // source term in the equation for nuq
360  Tenseur source_dzf(mp) ; // matter source term in the eq. for dzeta
361  Tenseur source_dzq(mp) ; // quadratic source term in the eq. for dzeta
362  Tenseur source_tggg(mp) ; // source term in the eq. for tggg
363  Tenseur source_shift(mp, 1, CON, mp.get_bvect_cart()) ;
364  // source term for shift
365  Tenseur mlngamma(mp) ; // centrifugal potential
366  Tenseur mlngamma2(mp) ; // centrifugal potential
367 
368  Tenseur *outer_ent_p; // pointer to the enthalpy field of the outer fluid
369 
370  // Preparations for the Poisson equations:
371  // --------------------------------------
372  if (nuf.get_etat() == ETATZERO) {
373  nuf.set_etat_qcq() ;
374  nuf.set() = 0 ;
375  }
376 
377  if (relativistic) {
378  if (nuq.get_etat() == ETATZERO) {
379  nuq.set_etat_qcq() ;
380  nuq.set() = 0 ;
381  }
382 
383  if (tggg.get_etat() == ETATZERO) {
384  tggg.set_etat_qcq() ;
385  tggg.set() = 0 ;
386  }
387 
388  if (dzeta.get_etat() == ETATZERO) {
389  dzeta.set_etat_qcq() ;
390  dzeta.set() = 0 ;
391  }
392  }
393 
394  ofstream fichconv("convergence.d") ; // Output file for diff_ent
395  fichconv << "# diff_ent GRV2 max_triax vit_triax" << endl ;
396 
397  ofstream fichfreq("frequency.d") ; // Output file for omega
398  fichfreq << "# f1 [Hz] f2 [Hz]" << endl ;
399 
400  ofstream fichevol("evolution.d") ; // Output file for various quantities
401  fichevol << "# r_pole/r_eq ent_c ent2_c" << endl ;
402 
403  diff_ent = 1 ;
404  double err_grv2 = 1 ;
405  double max_triax_prev = 0 ; // Triaxial amplitude at previous step
406 
407  //=========================================================================
408  // Start of iteration
409  //=========================================================================
410 
411  for(int mer=0 ; (diff_ent > precis) && (mer<mer_max) ; mer++ ) {
412 
413  cout << "-----------------------------------------------" << endl ;
414  cout << "step: " << mer << endl ;
415  cout << "diff_ent = " << display_bold << diff_ent << display_normal
416  << endl ;
417  cout << "err_grv2 = " << err_grv2 << endl ;
418  fichconv << mer ;
419  fichfreq << mer ;
420  fichevol << mer ;
421 
422  if (mer >= mer_rot) {
423 
424  if (mer < mer_change_omega) {
425  omega = omega_ini ;
426  omega2 = omega2_ini ;
427  }
428  else {
429  if (mer <= mer_fix_omega) {
430  omega = omega_ini + accrois_omega *
431  (mer - mer_change_omega) ;
432  omega2 = omega2_ini + accrois_omega2 *
433  (mer - mer_change_omega) ;
434  }
435  }
436 
437  }
438 
439  //-----------------------------------------------
440  // Sources of the Poisson equations
441  //-----------------------------------------------
442 
443  // Source for nu
444  // -------------
445  Tenseur beta = log(bbb) ;
446  beta.set_std_base() ;
447 
448  // common source term for relativistic and Newtonian ! (enerps_euler has the right limit)
449  source_nuf = qpig * a_car * enerps_euler;
450 
451  if (relativistic)
452  source_nuq = ak_car - flat_scalar_prod(logn.gradient_spher(),logn.gradient_spher() + beta.gradient_spher()) ;
453  else
454  source_nuq = 0 ;
455 
456  source_nuf.set_std_base() ;
457  source_nuq.set_std_base() ;
458 
459  if (relativistic) {
460  // Source for dzeta
461  // ----------------
462  source_dzf = 2 * qpig * a_car * sphph_euler;
463  source_dzf.set_std_base() ;
464 
465  source_dzq = 1.5 * ak_car - flat_scalar_prod(logn.gradient_spher(),logn.gradient_spher() ) ;
466  source_dzq.set_std_base() ;
467 
468  // Source for tggg
469  // ---------------
470 
471  source_tggg = 2 * qpig * nnn * a_car * bbb * (s_euler - sphph_euler);
472  source_tggg.set_std_base() ;
473 
474  (source_tggg.set()).mult_rsint() ;
475 
476 
477  // Source for shift
478  // ----------------
479 
480  // Matter term
481  source_shift = (-4*qpig) * nnn * a_car * j_euler;
482 
483  // Quadratic terms:
484  Tenseur vtmp = 3 * beta.gradient_spher() - logn.gradient_spher() ;
485  vtmp.change_triad(mp.get_bvect_cart()) ;
486 
487  Tenseur squad = 2 * nnn * flat_scalar_prod(tkij, vtmp) ;
488 
489  // The addition of matter terms and quadratic terms is performed
490  // component by component because u_euler is contravariant,
491  // while squad is covariant.
492 
493  if (squad.get_etat() == ETATQCQ) {
494  for (int i=0; i<3; i++) {
495  source_shift.set(i) += squad(i) ;
496  }
497  }
498 
499  source_shift.set_std_base() ;
500  }
501  //----------------------------------------------
502  // Resolution of the Poisson equation for nuf
503  //----------------------------------------------
504 
505  source_nuf().poisson(par_poisson_nuf, nuf.set()) ;
506 
507 // cout << "Test of the Poisson equation for nuf :" << endl ;
508 // Tbl err = source_nuf().test_poisson(nuf(), cout, true) ;
509 // diff_nuf = err(0, 0) ;
510  diff_nuf = 0 ;
511 
512  //---------------------------------------
513  // Triaxial perturbation of nuf
514  //---------------------------------------
515 
516  if (mer == mer_triax) {
517 
518  if ( mg->get_np(0) == 1 ) {
519  cout <<
520  "Et_rot_bifluid::equilibrium: np must be stricly greater than 1"
521  << endl << " to set a triaxial perturbation !" << endl ;
522  abort() ;
523  }
524 
525  const Coord& phi = mp.phi ;
526  const Coord& sint = mp.sint ;
527  Cmp perturb(mp) ;
528  perturb = 1 + ampli_triax * sint*sint * cos(2*phi) ;
529  nuf.set() = nuf() * perturb ;
530 
531  nuf.set_std_base() ; // set the bases for spectral expansions
532  // to be the standard ones for a
533  // scalar field
534 
535  }
536 
537  // Monitoring of the triaxial perturbation
538  // ---------------------------------------
539 
540  Valeur& va_nuf = nuf.set().va ;
541  va_nuf.coef() ; // Computes the spectral coefficients
542  double max_triax = 0 ;
543 
544  if ( mg->get_np(0) > 1 ) {
545 
546  for (int l=0; l<nz; l++) { // loop on the domains
547  for (int j=0; j<mg->get_nt(l); j++) {
548  for (int i=0; i<mg->get_nr(l); i++) {
549 
550  // Coefficient of cos(2 phi) :
551  double xcos2p = (*(va_nuf.c_cf))(l, 2, j, i) ;
552 
553  // Coefficient of sin(2 phi) :
554  double xsin2p = (*(va_nuf.c_cf))(l, 3, j, i) ;
555 
556  double xx = sqrt( xcos2p*xcos2p + xsin2p*xsin2p ) ;
557 
558  max_triax = ( xx > max_triax ) ? xx : max_triax ;
559  }
560  }
561  }
562  }
563  cout << "Triaxial part of nuf : " << max_triax << endl ;
564 
565  if (relativistic) {
566 
567  //----------------------------------------------
568  // Resolution of the Poisson equation for nuq
569  //----------------------------------------------
570 
571  source_nuq().poisson(par_poisson_nuq, nuq.set()) ;
572 
573 // cout << "Test of the Poisson equation for nuq :" << endl ;
574 // err = source_nuq().test_poisson(nuq(), cout, true) ;
575 // diff_nuq = err(0, 0) ;
576  diff_nuq = 0 ;
577 
578  //---------------------------------------------------------
579  // Resolution of the vector Poisson equation for the shift
580  //---------------------------------------------------------
581 
582  if (source_shift.get_etat() != ETATZERO) {
583 
584  for (int i=0; i<3; i++) {
585  if(source_shift(i).dz_nonzero()) {
586  assert( source_shift(i).get_dzpuis() == 4 ) ;
587  }
588  else{
589  (source_shift.set(i)).set_dzpuis(4) ;
590  }
591  }
592 
593  }
594 
595  double lambda_shift = double(1) / double(3) ;
596 
597  if ( mg->get_np(0) == 1 ) {
598  lambda_shift = 0 ;
599  }
600 
601  source_shift.poisson_vect(lambda_shift, par_poisson_vect,
602  shift, w_shift, khi_shift) ;
603 
604 // cout << "Test of the Poisson equation for shift_x :" << endl ;
605 // err = source_shift(0).test_poisson(shift(0), cout, true) ;
606 // diff_shift_x = err(0, 0) ;
607  diff_shift_x = 0 ;
608 
609 // cout << "Test of the Poisson equation for shift_y :" << endl ;
610 // err = source_shift(1).test_poisson(shift(1), cout, true) ;
611 // diff_shift_y = err(0, 0) ;
612  diff_shift_y = 0 ;
613 
614  // Computation of tnphi and nphi from the Cartesian components
615  // of the shift
616  // -----------------------------------------------------------
617 
618  fait_nphi() ;
619 
620  }
621 
622 
623  //----------------------------------------
624  // Shall we search for the Kepler limit?
625  //----------------------------------------
626  bool kepler = false;
627  bool too_fast = false;
628 
629  if ( (kepler_fluid > 0) && (mer > mer_fix_omega + kepler_wait_steps) )
630  {
631  if (kepler_fluid & 0x01)
632  omega *= kepler_factor;
633  if (kepler_fluid & 0x02)
634  omega2 *= kepler_factor;
635  }
636 
637 
638  // ============================================================
639  kepler = true;
640  while (kepler)
641  {
642 
643  // New computation of delta_car, gam_euler, enerps_euler etc...
644  // ------------------------------------------------------
645  hydro_euler() ;
646 
647 
648  //------------------------------------------------------
649  // First integral of motion
650  //------------------------------------------------------
651 
652  // Centrifugal potential :
653  if (relativistic) {
654  mlngamma = - log( gam_euler ) ;
655  mlngamma2 = - log( gam_euler2) ;
656  }
657  else {
658  mlngamma = - 0.5 * uuu*uuu ;
659  mlngamma2 = -0.5 * uuu2*uuu2 ;
660  }
661 
662  // Central values of various potentials :
663  double nuf_c = nuf()(0,0,0,0) ;
664  double nuq_c = nuq()(0,0,0,0) ;
665 
666  // Scale factor to ensure that the enthalpy is equal to ent_b at
667  // the equator for the "outer" fluid
668  double alpha_r2 = 0;
669 
670  int j=j_b;
671 
672  // Boundary values of various potentials :
673  double nuf_b = nuf()(l_b, k_b, j, i_b) ;
674  double nuq_b = nuq()(l_b, k_b, j, i_b) ;
675  double mlngamma_b = mlngamma()(l_b, k_b, j, i_b) ;
676  double mlngamma2_b = mlngamma2()(l_b, k_b, j, i_b) ;
677 
678 
679  // RP: "hack": adapt the radius correctly if using "slow-rot-style" EOS inversion
680  //
681  if ( eos.identify() == 2 ) // only applies to Eos_bf_poly_newt
682  {
683  const Eos_bf_poly_newt &eos0 = dynamic_cast<const Eos_bf_poly_newt&>(eos);
684  if (eos0.get_typeos() == 5)
685  {
686  double vn_b = uuu()(l_b, k_b, j, i_b);
687  double vp_b = uuu2()(l_b, k_b, j, i_b);
688  double D2_b = (vp_b - vn_b)*(vp_b - vn_b);
689  double kdet = eos0.get_kap3() + eos0.get_beta()*D2_b;
690  double kaps1 = kdet / ( eos0.get_kap2() - kdet );
691  double kaps2 = kdet / ( eos0.get_kap1() - kdet );
692 
693  ent1_b = kaps1 * ( ent2_c - ent_c - mlngamma2_b + mlngamma_b );
694  ent2_b = kaps2 * ( ent_c - ent2_c - mlngamma_b + mlngamma2_b );
695 
696  cout << "**********************************************************************\n";
697  cout << "DEBUG: Rescaling domain for slow-rot-style EOS inversion \n";
698  cout << "DEBUG: ent1_b = " << ent1_b << "; ent2_b = " << ent2_b << endl;
699  cout << "**********************************************************************\n";
700 
701  adapt_flag = 0; // don't do adaptive-grid if using slow-rot-style inversion!
702  }
703  }
704 
705  double alpha1_r2 = ( ent_c - ent1_b - mlngamma_b + nuq_c - nuq_b) / ( nuf_b - nuf_c ) ;
706  double alpha2_r2 = ( ent2_c - ent2_b - mlngamma2_b + nuq_c - nuq_b) / ( nuf_b - nuf_c ) ;
707 
708  cout << "DEBUG: j= "<< j<<" ; alpha1 = " << alpha1_r2 <<" ; alpha2 = " << alpha2_r2 << endl;
709 
710  int outer_fluid = (alpha1_r2 > alpha2_r2) ? 1 : 2; // index of 'outer' fluid (at equator!)
711 
712  outer_ent_p = (outer_fluid == 1) ? (&ent) : (&ent2);
713 
714  alpha_r2 = (outer_fluid == 1) ? alpha1_r2 : alpha2_r2 ;
715 
716  alpha_r = sqrt(alpha_r2);
717 
718  cout << "alpha_r = " << alpha_r << endl ;
719 
720  // Readjustment of nu :
721  // -------------------
722 
723  logn = alpha_r2 * nuf + nuq ;
724  double nu_c = logn()(0,0,0,0) ;
725 
726 
727  // First integral --> enthalpy in all space
728  //-----------------
729 
730  ent = (ent_c + nu_c) - logn - mlngamma ;
731  ent2 = (ent2_c + nu_c) - logn - mlngamma2 ;
732 
733 
734  // now let's try to figure out if we have overstepped the Kepler-limit
735  // (FIXME) we assume that the enthalpy of the _outer_ fluid being negative
736  // inside the star
737  kepler = false;
738  for (int l=0; l<nzet; l++) {
739  int imax = mg->get_nr(l) - 1 ;
740  if (l == l_b) imax-- ; // The surface point is skipped
741  for (int i=0; i<imax; i++) {
742  if ( (*outer_ent_p)()(l, 0, j_b, i) < 0. ) {
743  kepler = true;
744  cout << "(outer) ent < 0 for l, i : " << l << " " << i
745  << " ent = " << (*outer_ent_p)()(l, 0, j_b, i) << endl ;
746  }
747  }
748  }
749 
750  if ( kepler )
751  {
752  cout << "**** KEPLERIAN VELOCITY REACHED ****" << endl ;
753  if (kepler_fluid & 0x01)
754  omega /= kepler_factor ; // Omega is decreased
755  if (kepler_fluid & 0x02)
756  omega2 /= kepler_factor;
757 
758  cout << "New rotation frequencies : "
759  << "Omega = " << omega/(2.*M_PI) * f_unit << " Hz; "
760  << "Omega2 = " << omega2/(2.*M_PI) * f_unit << endl ;
761 
762  too_fast = true;
763  }
764 
765  } /* while kepler */
766 
767 
768  if ( too_fast )
769  { // fact_omega is decreased for the next step
770  kepler_factor = sqrt( kepler_factor ) ;
771  cout << "**** New fact_omega : " << kepler_factor << endl ;
772  }
773  // ============================================================
774 
775 
776  // Cusp-check: shall the adaptation still be performed?
777  // ------------------------------------------
778  double dent_eq = (*outer_ent_p)().dsdr()(l_b, k_b, j_b, i_b) ;
779  double dent_pole = (*outer_ent_p)().dsdr()(l_b, k_b, 0, i_b) ;
780  double rap_dent = fabs( dent_eq / dent_pole ) ;
781  cout << "| dH/dr_eq / dH/dr_pole | = " << rap_dent << endl ;
782 
783  if ( rap_dent < thres_adapt ) {
784  adapt_flag = 0 ; // No adaptation of the mapping
785  cout << "******* FROZEN MAPPING *********" << endl ;
786  }
787 
788  // Rescaling of the grid and adaption to (outer) enthalpy surface
789  //---------------------------------------
790  if (adapt_flag && (nzadapt > 0) )
791  {
792  mp_prev = mp_et ;
793 
794  mp.adapt( (*outer_ent_p)(), par_adapt) ;
795 
796  mp_prev.homothetie(alpha_r) ;
797 
798  mp.reevaluate(&mp_prev, nzet+1, ent.set()) ;
799  mp.reevaluate(&mp_prev, nzet+1, ent2.set()) ;
800  }
801  else
802  mp.homothetie (alpha_r);
803 
804 
805  //----------------------------------------------------
806  // Equation of state
807  //----------------------------------------------------
808 
809  equation_of_state() ; // computes new values for nbar1,2 , ener (e)
810  // and press (p) from the new ent,ent2
811 
812  //---------------------------------------------------------
813  // Matter source terms in the gravitational field equations
814  //---------------------------------------------------------
815 
816  //## Computation of tnphi and nphi from the Cartesian components
817  // of the shift for the test in hydro_euler():
818 
819  fait_nphi() ;
820 
821  hydro_euler() ; // computes new values for ener_euler (E),
822  // s_euler (S) and u_euler (U^i)
823 
824  if (relativistic) {
825 
826  //-------------------------------------------------------
827  // 2-D Poisson equation for tggg
828  //-------------------------------------------------------
829 
830  mp.poisson2d(source_tggg(), mp.cmp_zero(), par_poisson_tggg, tggg.set()) ;
831 
832  //-------------------------------------------------------
833  // 2-D Poisson equation for dzeta
834  //-------------------------------------------------------
835 
836  mp.poisson2d(source_dzf(), source_dzq(), par_poisson_dzeta, dzeta.set()) ;
837 
838  err_grv2 = lbda_grv2 - 1;
839  cout << "GRV2: " << err_grv2 << endl ;
840 
841  }
842  else {
843  err_grv2 = grv2() ;
844  }
845 
846 
847  //---------------------------------------
848  // Computation of the metric coefficients (except for N^phi)
849  //---------------------------------------
850 
851  // Relaxations on nu and dzeta :
852 
853  if (mer >= 10) {
854  logn = relax * logn + relax_prev * logn_prev ;
855 
856  dzeta = relax * dzeta + relax_prev * dzeta_prev ;
857  }
858 
859  // Update of the metric coefficients N, A, B and computation of K_ij :
860 
861  update_metric() ;
862 
863  //-----------------------
864  // Informations display
865  //-----------------------
866 
867  // partial_display(cout) ;
868  fichfreq << " " << omega / (2*M_PI) * f_unit ;
869  fichfreq << " " << omega2 / (2*M_PI) * f_unit ;
870  fichevol << " " << ray_pole() / ray_eq() ;
871  fichevol << " " << ent_c ;
872  fichevol << " " << ent2_c ;
873 
874 
875  //-----------------------------------------
876  // Convergence towards given baryon masses (if mer_mass > 0)
877  //-----------------------------------------
878 
879 
880  cout << "DEBUG MODE : mbar1_wanted : " << mbar1_wanted/msol << endl ;
881  cout << "DEBUG MODE : mbar2_wanted : " << mbar2_wanted/msol << endl ;
882 
883  // If we want to impose baryonic masses for both fluids.
884  // Be careful, the code acts on mu_n and mu_p (at the center)
885  // -> beta equilibrium can be not verified
886  // CV towards Mbn and Mbp (without beta equilibrium at the center)
887  if (mbar2_wanted > 0 )
888  {
889  if ((mer_mass>0) && (mer > mer_mass)) {
890 
891  double xx, xprog, ax, fact;
892 
893  // fluid 1
894  xx = mass_b1() / mbar1_wanted - 1. ;
895  cout << "Discrep. baryon mass1 <-> wanted bar. mass1 : " << xx << endl ;
896 
897  xprog = ( mer > 2*mer_mass) ? 1. : double(mer - mer_mass)/double(mer_mass) ;
898  xx *= xprog ;
899  ax = 0.5 * ( 2. + xx ) / (1. + xx ) ;
900  fact = pow(ax, aexp_mass) ;
901  cout << "Fluid1: xprog, xx, ax, fact : " << xprog << " " << xx << " " << ax << " " << fact << endl ;
902  ent_c *= fact ;
903 
904  // fluid 2
905  xx = mass_b2() / mbar2_wanted - 1. ;
906  cout << "Discrep. baryon mass2 <-> wanted bar. mass2 : " << xx << endl ;
907 
908  xprog = ( mer > 2*mer_mass) ? 1. : double(mer - mer_mass)/double(mer_mass) ;
909  xx *= xprog ;
910  ax = 0.5 * ( 2. + xx ) / (1. + xx ) ;
911  fact = pow(ax, aexp_mass) ;
912  cout << "Fluid2: xprog, xx, ax, fact : " << xprog << " " << xx << " " << ax << " " << fact << endl ;
913  ent2_c *= fact ;
914  cout << "H1c = " << ent_c << " H2c = " << ent2_c << endl ;
915  }
916  }
917 
918  // CV towards a given GRAVITATIONAL mass (with beta-eq at the center)
919  else if (mbar2_wanted/msol == -1. ) {
920 
921  if ((mer_mass>0) && (mer > mer_mass)) {
922 
923  double xx, xprog, ax, fact;
924 
925  // total mass
926  xx = mass_g() / mbar1_wanted - 1. ; // mbar1_wanted = "mgrav_wanted"
927  cout << "Discrep. baryon mass <-> wanted bar. mass : " << xx << endl ;
928 
929  xprog = ( mer > 2*mer_mass) ? 1. : double(mer - mer_mass)/double(mer_mass) ;
930  xx *= xprog ;
931  ax = 0.5 * ( 2. + xx ) / (1. + xx ) ;
932  fact = pow(ax, aexp_mass) ;
933  cout << "Fluid1: xprog, xx, ax, fact : " << xprog << " " << xx << " " << ax << " " << fact << endl ;
934  ent_c *= fact ;
935 
936  double m1 = eos.get_m1() ;
937  double m2 = eos.get_m2() ;
938  cout << "m1 = " << m1 << " m2 = " << m2 << endl;
939  ent2_c = ent_c + log(m1/m2); // to ensure beta_equilibrium at the center
940  cout << "DEBUG MODE : ent_c " << ent_c << endl ;
941  cout << "DEBUG MODE : ent2_c " << ent2_c << endl ;
942  cout << "H1c = " << ent_c << " H2c = " << ent2_c << endl ;
943 
944  }
945  }
946  // If we want to impose Mb_tot and beta equilibrium (at the center)
947  // In this case : mbar1_wanted = total baryonic mass wanted
948  // mbar2_wanted should be set to 0 and is not used.
949  else {
950 
951  if ((mer_mass>0) && (mer > mer_mass)) {
952 
953  double xx, xprog, ax, fact;
954 
955  // total mass
956  xx = mass_b() / mbar1_wanted - 1. ; // mbar1_wanted = " mbar_wanted"
957  cout << "Discrep. baryon mass <-> wanted bar. mass : " << xx << endl ;
958 
959  xprog = ( mer > 2*mer_mass) ? 1. : double(mer - mer_mass)/double(mer_mass) ;
960  xx *= xprog ;
961  ax = 0.5 * ( 2. + xx ) / (1. + xx ) ;
962  fact = pow(ax, aexp_mass) ;
963  cout << "Fluid1: xprog, xx, ax, fact : " << xprog << " " << xx << " " << ax << " " << fact << endl ;
964  ent_c *= fact ;
965 
966  double m1 = eos.get_m1() ;
967  double m2 = eos.get_m2() ;
968  cout << "m1 = " << m1 << " m2 = " << m2 << endl;
969  ent2_c = ent_c + log(m1/m2); // to ensure beta_equilibrium at the center
970  cout << "DEBUG MODE : ent_c " << ent_c << endl ;
971  cout << "DEBUG MODE : ent2_c " << ent2_c << endl ;
972  cout << "H1c = " << ent_c << " H2c = " << ent2_c << endl ;
973 
974  }
975 
976  } /* if mer > mer_mass */
977 
978 
979  //-------------------------------------------------------------
980  // Relative change in enthalpies with respect to previous step
981  //-------------------------------------------------------------
982 
983  Tbl diff_ent_tbl = diffrel( ent(), ent_prev() ) ;
984  diff_ent1 = diff_ent_tbl(0) ;
985  for (int l=1; l<nzet; l++) {
986  diff_ent1 += diff_ent_tbl(l) ;
987  }
988  diff_ent1 /= nzet ;
989  diff_ent_tbl = diffrel( ent2(), ent2_prev() ) ;
990  diff_ent2 = diff_ent_tbl(0) ;
991  for (int l=1; l<nzet; l++) {
992  diff_ent2 += diff_ent_tbl(l) ;
993  }
994  diff_ent2 /= nzet ;
995  diff_ent = 0.5*(diff_ent1 + diff_ent2) ;
996 
997  fichconv << " " << log10( fabs(diff_ent) + 1.e-16 ) ;
998  fichconv << " " << log10( fabs(err_grv2) + 1.e-16 ) ;
999  fichconv << " " << log10( fabs(max_triax) + 1.e-16 ) ;
1000 
1001  vit_triax = 0 ;
1002  if ( (mer > mer_triax+1) && (max_triax_prev > 1e-13) ) {
1003  vit_triax = (max_triax - max_triax_prev) / max_triax_prev ;
1004  }
1005 
1006  fichconv << " " << vit_triax ;
1007 
1008  //------------------------------
1009  // Recycling for the next step
1010  //------------------------------
1011 
1012  ent_prev = ent ;
1013  ent2_prev = ent2 ;
1014  logn_prev = logn ;
1015  dzeta_prev = dzeta ;
1016  max_triax_prev = max_triax ;
1017 
1018  fichconv << endl ;
1019  fichfreq << endl ;
1020  fichevol << endl ;
1021  fichconv.flush() ;
1022  fichfreq.flush() ;
1023  fichevol.flush() ;
1024 
1025  } // End of main loop
1026 
1027  //=========================================================================
1028  // End of iteration
1029  //=========================================================================
1030 
1031  fichconv.close() ;
1032  fichfreq.close() ;
1033  fichevol.close() ;
1034 
1035 
1036 }
1037 
1038 }
Cmp log(const Cmp &)
Neperian logarithm.
Definition: cmp_math.C:299
Mtbl_cf * c_cf
Coefficients of the spectral expansion of the function.
Definition: valeur.h:312
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
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
const Tenseur & gradient_spher() const
Returns the gradient of *this (Spherical coordinates) (scalar field only).
Definition: tenseur.C:1564
int get_np(int l) const
Returns the number of points in the azimuthal direction ( ) in domain no. l.
Definition: grilles.h:479
void coef() const
Computes the coeffcients of *this.
Definition: valeur_coef.C:151
Cmp sqrt(const Cmp &)
Square root.
Definition: cmp_math.C:223
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
double get_kap2() const
Returns the pressure coefficient [unit: ], where .
Definition: eos_bifluid.h:941
Standard units of space, time and mass.
double & set(int i)
Read/write of a particular element (index i) (1D case)
Definition: tbl.h:301
Tenseur flat_scalar_prod(const Tenseur &t1, const Tenseur &t2)
Scalar product of two Tenseur when the metric is : performs the contraction of the last index of t1 w...
int get_type_t() const
Returns the type of sampling in the direction: SYM : : symmetry with respect to the equatorial pl...
Definition: grilles.h:502
double get_kap3() const
Returns the pressure coefficient [unit: ], where .
Definition: eos_bifluid.h:947
Basic integer array class.
Definition: itbl.h:122
Values and coefficients of a (real-value) function.
Definition: valeur.h:297
Cmp cos(const Cmp &)
Cosine.
Definition: cmp_math.C:97
Tbl diffrel(const Cmp &a, const Cmp &b)
Relative difference between two Cmp (norme version).
Definition: cmp_math.C:507
void add_double_mod(double &x, int position=0)
Adds the address of a new modifiable double to the list.
Definition: param.C:456
void set_etat_qcq()
Sets the logical state to ETATQCQ (ordinary state).
Definition: tbl.C:364
Cmp & set()
Read/write for a scalar (see also operator=(const Cmp&) ).
Definition: tenseur.C:840
void change_triad(const Base_vect &new_triad)
Sets a new vectorial basis (triad) of decomposition and modifies the components accordingly.
Definition: tenseur.C:684
double get_kap1() const
Returns the pressure coefficient [unit: ], where .
Definition: eos_bifluid.h:935
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
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
Analytic equation of state for two fluids (Newtonian case).
Definition: eos_bifluid.h:1161
int get_etat() const
Returns the logical state.
Definition: tenseur.h:710
Cmp pow(const Cmp &, int)
Power .
Definition: cmp_math.C:351
Active physical coordinates and mapping derivatives.
Definition: coord.h:90
int get_nr(int l) const
Returns the number of points in the radial direction ( ) in domain no. l.
Definition: grilles.h:469
Multi-domain grid.
Definition: grilles.h:279
virtual void adapt(const Cmp &ent, const Param &par, int nbr_filtre=0)
Adaptation of the mapping to a given scalar field.
Definition: map_et_adapt.C:111
Cmp log10(const Cmp &)
Basis 10 logarithm.
Definition: cmp_math.C:325
double get_beta() const
Returns the coefficient [unit: ], where .
Definition: eos_bifluid.h:953
void add_double(const double &x, int position=0)
Adds the the address of a new double to the list.
Definition: param.C:318
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
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 equilibrium_bi(double ent_c, double ent_c2, double omega0, double omega20, const Tbl &ent_limit, const Tbl &ent2_limit, const Itbl &icontrol, const Tbl &control, Tbl &diff, int mer_mass, double mbar1_wanted, double mbar2_wanted, double aexp_mass)
Computes an equilibrium configuration.
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
Tbl & set(int l)
Read/write of the value in a given domain (configuration space).
Definition: valeur.h:373