LORENE
binaire_ana_shift.C
1/*
2 * Method of class Binaire to set some analytical form to the shift vector.
3 *
4 * (see file binaire.h for documentation).
5 */
6
7/*
8 * Copyright (c) 2000-2001 Eric Gourgoulhon
9 * Copyright (c) 2000-2001 Keisuke Taniguchi
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: binaire_ana_shift.C,v 1.4 2016/12/05 16:17:47 j_novak Exp $
34 * $Log: binaire_ana_shift.C,v $
35 * Revision 1.4 2016/12/05 16:17:47 j_novak
36 * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
37 *
38 * Revision 1.3 2014/10/13 08:52:44 j_novak
39 * Lorene classes and functions now belong to the namespace Lorene.
40 *
41 * Revision 1.2 2004/03/25 10:28:59 j_novak
42 * All LORENE's units are now defined in the namespace Unites (in file unites.h).
43 *
44 * Revision 1.1.1.1 2001/11/20 15:19:30 e_gourgoulhon
45 * LORENE
46 *
47 * Revision 2.3 2000/03/17 15:36:26 eric
48 * Suppression de l'appel a analytical_omega().
49 *
50 * Revision 2.2 2000/03/17 15:27:11 eric
51 * Appel de la fonction analytical_omega() pour fixer la valeur de omega.
52 *
53 * Revision 2.1 2000/03/16 09:37:28 eric
54 * Utilisation du cas incompressible plutot que n=1.
55 *
56 * Revision 2.0 2000/03/15 16:43:35 eric
57 * *** empty log message ***
58 *
59 *
60 * $Header: /cvsroot/Lorene/C++/Source/Binaire/binaire_ana_shift.C,v 1.4 2016/12/05 16:17:47 j_novak Exp $
61 *
62 */
63
64// Headers C
65#include "math.h"
66
67// Headers Lorene
68#include "binaire.h"
69#include "unites.h"
70
71namespace Lorene {
73
74 // Does nothing for a Newtonian star
75 // ---------------------------------
76 if ( !star1.is_relativistic() ){
77 assert( !star2.is_relativistic() ) ;
78 return ;
79 }
80
81
82 using namespace Unites ;
83
84 for (int i=0; i<2; i++) {
85
86 // Radius of the star:
87 double a0 = et[i]->ray_eq() ;
88
89 // Mass ratio
90 double p_mass = et[i]->mass_g() / et[1-i]->mass_g() ;
91
92 // G M Omega R / (1+p)
93 double www = ggrav * et[i]->mass_g() * omega
94 * separation() / (1. + p_mass) ;
95
96 const Map& mp = et[i]->get_mp() ;
97 Cmp tmp(mp) ;
98 Cmp tmp_ext(mp) ;
99 int nzet = et[i]->get_nzet() ;
100 int nzm1 = mp.get_mg()->get_nzone() - 1 ;
101
102 // Computation of w_shift
103 // ----------------------
104 et[i]->set_w_shift().set_etat_qcq() ;
105
106 // X component
107 // -----------
108 et[i]->set_w_shift().set(0) = 0 ;
109
110 // Y component
111 // -----------
112
113// For the incompressible case :
114 tmp = - 6 * www / a0 * ( 1 - (mp.r)*(mp.r) / (3*a0*a0) ) ;
115
116// For the compressible (n=1) case :
117// Mtbl xi = M_PI * mp.r / a0 ;
118// Mtbl sinc = sin(xi) / xi ;
119// The value of sinc is set to 1 at the origin
120// for (int k=0; k<mp.get_mg()->get_np(0); k++) {
121// for (int j=0; j<mp.get_mg()->get_nt(0); j++) {
122// sinc.set(0, k, j, 0) = 1 ;
123// }
124// }
125// tmp = - 4 * www / a0 * ( 1 + sinc ) ;
126
127 tmp.annule(nzet, nzm1) ;
128 tmp_ext = - 4 * www / mp.r ;
129 tmp_ext.annule(0, nzet-1) ;
130
131 et[i]->set_w_shift().set(1) = tmp + tmp_ext ;
132
133 // Z component
134 // -----------
135 et[i]->set_w_shift().set(2) = 0 ;
136
137 // Sets the standard spectral bases for Cartesian components
138 et[i]->set_w_shift().set_std_base() ;
139
140 // Computation of khi_shift
141 // ------------------------
142
143 tmp = 2 * www / a0 * (mp.y) * ( 1 - 3 * (mp.r)*(mp.r) / (5*a0*a0) ) ;
144 tmp.annule(nzet, nzm1) ;
145 tmp_ext = 0.8 * www * a0*a0 * (mp.sint) * (mp.sinp)
146 / (mp.r * mp.r) ;
147 tmp_ext.annule(0, nzet-1) ;
148
149 et[i]->set_khi_shift() = tmp + tmp_ext ;
150
151 // Sets the standard spectral bases for a scalar field
152 et[i]->set_khi_shift().set_std_base() ;
153
154 }
155
156}
157}
void analytical_shift()
Sets some analytical template for the shift vector (via the members {\tt w_shift} and {\tt khi_shift}...
Etoile_bin * et[2]
Array of the two stars (to perform loops on the stars): {\tt et[0]} contains the address of {\tt star...
Definition binaire.h:127
double separation() const
Returns the coordinate separation of the two stellar centers [{\tt r_unit}].
Definition binaire.C:460
Etoile_bin star2
Second star of the system.
Definition binaire.h:121
double omega
Angular velocity with respect to an asymptotically inertial observer.
Definition binaire.h:132
Etoile_bin star1
First star of the system.
Definition binaire.h:118
Component of a tensorial field *** DEPRECATED : use class Scalar instead ***.
Definition cmp.h:446
void annule(int l)
Sets the Cmp to zero in a given domain.
Definition cmp.C:351
Lorene prototypes.
Definition app_hor.h:67
Map(const Mg3d &)
Constructor from a multi-domain 3D grid.
Definition map.C:142
Standard units of space, time and mass.