LORENE
binary_omegaana.C
1/*
2 * Methods of class Binary to set analytical value to omega
3 *
4 */
5
6/*
7 * Copyright (c) 2004 Francois Limousin
8 *
9 * This file is part of LORENE.
10 *
11 * LORENE is free software; you can redistribute it and/or modify
12 * it under the terms of the GNU General Public License as published by
13 * the Free Software Foundation; either version 2 of the License, or
14 * (at your option) any later version.
15 *
16 * LORENE is distributed in the hope that it will be useful,
17 * but WITHOUT ANY WARRANTY; without even the implied warranty of
18 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
19 * GNU General Public License for more details.
20 *
21 * You should have received a copy of the GNU General Public License
22 * along with LORENE; if not, write to the Free Software
23 * Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA
24 *
25 */
26
27
28
29
30/*
31 * $Id: binary_omegaana.C,v 1.5 2016/12/05 16:17:47 j_novak Exp $
32 * $Log: binary_omegaana.C,v $
33 * Revision 1.5 2016/12/05 16:17:47 j_novak
34 * Suppression of some global variables (file names, loch, ...) to prevent redefinitions
35 *
36 * Revision 1.4 2014/10/13 08:52:45 j_novak
37 * Lorene classes and functions now belong to the namespace Lorene.
38 *
39 * Revision 1.3 2004/03/25 10:29:01 j_novak
40 * All LORENE's units are now defined in the namespace Unites (in file unites.h).
41 *
42 * Revision 1.2 2004/01/20 15:21:52 f_limousin
43 * First version
44 *
45 *
46 * $Header: /cvsroot/Lorene/C++/Source/Binary/binary_omegaana.C,v 1.5 2016/12/05 16:17:47 j_novak Exp $
47 *
48 */
49
50// Headers C
51#include "math.h"
52
53// Headers Lorene
54#include "binary.h"
55#include "unites.h"
56
57
58namespace Lorene {
60
61 using namespace Unites ;
62
63 double rr = separation() ;
64 double mtot = star1.mass_g() + star2.mass_g() ;
65
66 // Compacity factor
67 double compact = ggrav * mtot / rr ;
68
69 double omega2 ;
70
71 if ( star1.is_irrotational() ) {
72
73 // Irrotational case
74 // -----------------
75
76 assert( star2.is_irrotational() ) ;
77
78 omega2 = ggrav * mtot / pow(rr, 3)
79 * (1. - 2.75 * compact + 8.625 * compact*compact ) ;
80
81 }
82 else{ // Corotating case
83 // ---------------
84
85 assert( !star2.is_irrotational() ) ;
86
87 // a0/R
88 double a0sr = star1.ray_eq() / rr ;
89
90 // Rescaled moment of inertia 5 I / (2 M a0^2)
91 double ired = double(5)/double(3) * ( 1. - double(6) / M_PI / M_PI ) ;
92 omega2 = ggrav * mtot / pow(rr, 3)
93 * (1. - compact * ( 2.75 + 2.*a0sr*a0sr * ired
94 - 0.48*pow(a0sr, 4) * ired*ired )
95 + compact*compact * ( 8.625 + 2.75*a0sr*a0sr * ired
96 + 2.*pow(a0sr, 4) * ired*ired ) ) ;
97
98 }
99
100 omega = sqrt( omega2 ) ;
101
102 // The derived quantities are obsolete:
103 del_deriv() ;
104
105}
106}
void del_deriv() const
Deletes all the derived quantities.
Definition binary.C:167
double omega
Angular velocity with respect to an asymptotically inertial observer.
Definition binary.h:94
void analytical_omega()
Sets the orbital angular velocity to some 2-PN analytical value (Keplerian value in the Newtonian cas...
Star_bin star2
Second star of the system.
Definition binary.h:83
Star_bin star1
First star of the system.
Definition binary.h:80
double separation() const
Returns the coordinate separation of the two stellar centers [r_unit].
Definition binary.C:610
Cmp sqrt(const Cmp &)
Square root.
Definition cmp_math.C:223
Cmp pow(const Cmp &, int)
Power .
Definition cmp_math.C:351
Lorene prototypes.
Definition app_hor.h:67
Standard units of space, time and mass.