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/*
* Methods of class Bin_bhns_extr
*
* (see file bin_bhns_extr.h for documentation).
*
*/
/*
* Copyright (c) 2004-2005 Keisuke Taniguchi
*
* 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 bin_bhns_extr_C[] = "$Header: /cvsroot/Lorene/C++/Source/Bin_bhns_extr/bin_bhns_extr.C,v 1.10 2014/10/13 08:52:41 j_novak Exp $" ;
/*
* $Id: bin_bhns_extr.C,v 1.10 2014/10/13 08:52:41 j_novak Exp $
* $Log: bin_bhns_extr.C,v $
* Revision 1.10 2014/10/13 08:52:41 j_novak
* Lorene classes and functions now belong to the namespace Lorene.
*
* Revision 1.9 2014/10/06 15:13:00 j_novak
* Modified #include directives to use c++ syntax.
*
* Revision 1.8 2005/02/28 23:06:16 k_taniguchi
* Modification of some arguments to include the case of the conformally
* flat background metric.
*
* Revision 1.7 2004/12/13 21:08:59 k_taniguchi
* Addition of some outputs in display_poly.
*
* Revision 1.6 2004/12/03 20:17:52 k_taniguchi
* Correction of "display_poly">
*
* Revision 1.5 2004/12/02 22:43:35 k_taniguchi
* Modification of "display_poly".
*
* Revision 1.4 2004/12/02 17:36:42 k_taniguchi
* Modification of "display_poly()".
*
* Revision 1.3 2004/12/01 16:37:11 k_taniguchi
* Modification of the output again.
*
* Revision 1.2 2004/12/01 16:27:09 k_taniguchi
* Modification of the output.
*
* Revision 1.1 2004/11/30 20:45:49 k_taniguchi
* *** empty log message ***
*
*
* $Header: /cvsroot/Lorene/C++/Source/Bin_bhns_extr/bin_bhns_extr.C,v 1.10 2014/10/13 08:52:41 j_novak Exp $
*
*/
// C headers
#include <cmath>
// Lorene headers
#include "bin_bhns_extr.h"
#include "eos.h"
#include "utilitaires.h"
#include "unites.h"
//--------------------------------//
// Constructors //
//--------------------------------//
// Standard constructor
// --------------------
namespace Lorene {
Bin_bhns_extr::Bin_bhns_extr(Map& mp, int nzet, const Eos& eos, bool irrot,
bool relat, bool kerrs, bool multi)
: ref_triad(0., "Absolute frame Cartesian basis"),
star(mp, nzet, relat, eos, irrot, ref_triad, kerrs, multi)
{
omega = 0. ;
separ = 0. ;
mass_bh = 0. ;
// Pointers of derived quantities initialized to zero :
set_der_0x0() ;
}
// Copy constructor
// ----------------
Bin_bhns_extr::Bin_bhns_extr(const Bin_bhns_extr& bibi)
: ref_triad(0., "Absolute frame Cartesian basis"),
star(bibi.star),
omega(bibi.omega),
separ(bibi.separ),
mass_bh(bibi.mass_bh)
{
// Pointers of derived quantities initialized to zero :
set_der_0x0() ;
}
// Constructor from a file
// -----------------------
Bin_bhns_extr::Bin_bhns_extr(Map& mp, const Eos& eos, FILE* fich)
: ref_triad(0., "Absolute frame Cartesian basis"),
star(mp, eos, ref_triad, fich)
{
// omega and x_axe are read in the file :
fread_be(&omega, sizeof(double), 1, fich) ;
fread_be(&separ, sizeof(double), 1, fich) ;
fread_be(&mass_bh, sizeof(double), 1, fich) ;
// Pointers of derived quantities initialized to zero :
set_der_0x0() ;
}
//------------------------------//
// Destructor //
//------------------------------//
Bin_bhns_extr::~Bin_bhns_extr()
{
del_deriv() ;
}
//----------------------------------------------------//
// Management of derived quantities //
//----------------------------------------------------//
void Bin_bhns_extr::del_deriv() const {
if (p_xa_barycenter_extr != 0x0) delete p_xa_barycenter_extr ;
if (p_ya_barycenter_extr != 0x0) delete p_ya_barycenter_extr ;
if (p_mass_b_extr != 0x0) delete p_mass_b_extr ;
set_der_0x0() ;
}
void Bin_bhns_extr::set_der_0x0() const {
p_xa_barycenter_extr = 0x0 ;
p_ya_barycenter_extr = 0x0 ;
p_mass_b_extr = 0x0 ;
}
//------------------------------//
// Assignment //
//------------------------------//
// Assignment to another Bin_bhns_extr
// -----------------------------------
void Bin_bhns_extr::operator=(const Bin_bhns_extr& bibi) {
assert( bibi.ref_triad == ref_triad ) ;
star = bibi.star ;
omega = bibi.omega ;
separ = bibi.separ ;
mass_bh = bibi.mass_bh ;
// ref_triad remains unchanged
del_deriv() ; // Deletes all derived quantities
}
//---------------------------//
// Outputs //
//---------------------------//
// Save in a file
// --------------
void Bin_bhns_extr::sauve(FILE* fich) const {
star.sauve(fich) ;
fwrite_be(&omega, sizeof(double), 1, fich) ;
fwrite_be(&separ, sizeof(double), 1, fich) ;
fwrite_be(&mass_bh, sizeof(double), 1, fich) ;
}
// Printing
// --------
ostream& operator<<(ostream& ost, const Bin_bhns_extr& bibi) {
bibi >> ost ;
return ost ;
}
ostream& Bin_bhns_extr::operator>>(ostream& ost) const {
using namespace Unites ;
ost << endl ;
ost << "Binary BH-NS system" << endl ;
ost << "===================" << endl ;
ost << endl ;
if (star.in_kerrschild()) {
ost << "Kerr-Schild background metric" << endl ;
ost << "-----------------------------" << endl ;
}
else {
ost << "Conformally flat background metric" << endl ;
ost << "----------------------------------" << endl ;
}
if (star.with_multipole()) {
ost << "Multipole falloff boundary condition" << endl ;
ost << "------------------------------------" << endl ;
}
else {
ost << "1/r falloff boundary condition" << endl ;
ost << "------------------------------" << endl ;
}
ost << endl
<< "Orbital angular velocity : "
<< omega * f_unit << " rad/s" << endl ;
ost << "Coordinate separation between BH and NS : "
<< separ / km << " km" << endl ;
ost << endl << "Neutron star : " ;
ost << endl << "============ " << endl ;
ost << endl ;
if (star.is_relativistic()) {
ost << "Relativistic star" << endl ;
ost << "-----------------" << endl ;
}
else {
ost << "WARNING : BH-NS binary should be relativistic !!!" << endl ;
ost << "-------------------------------------------------" << endl ;
}
ost << "Number of domains occupied by the star : " << star.get_nzet()
<< endl ;
ost << "Equation of state : " << endl ;
ost << star.get_eos() << endl ;
ost << endl
<< "Enthalpy at the coordinate origin : "
<< star.get_ent()()(0,0,0,0) << " c^2" << endl ;
ost << "Proper baryon density at the coordinate origin : "
<< star.get_nbar()()(0,0,0,0) << " x 0.1 fm^-3" << endl ;
ost << "Proper energy density at the coordinate origin : "
<< star.get_ener()()(0,0,0,0) << " rho_nuc c^2" << endl ;
ost << "Pressure at the coordinate origin : "
<< star.get_press()()(0,0,0,0) << " rho_nuc c^2" << endl ;
ost << endl
<< "Lapse N at the coordinate origin : "
<< star.get_nnn()()(0,0,0,0) << endl ;
ost << "Conformal factor A^2 at the coordinate origin : "
<< star.get_a_car()()(0,0,0,0) << endl ;
ost << endl
<< "Equatorial radius (to BH) a_to : "
<< star.ray_eq_pi()/km << " km" << endl ;
ost << "Equatorial radius (opp. to BH) a_opp : "
<< star.ray_eq()/km << " km" << endl ;
ost << endl
<< "Baryon mass in isolation : " << star.mass_b() / msol
<< " Mo" << endl
<< "Gravitational mass in isolation : " << star.mass_g() / msol
<< " Mo" << endl
<< "Baryon mass in a binary system : " << mass_b_extr() / msol
<< " Mo" << endl ;
ost << endl ;
ost << "Star in a binary system" << endl ;
ost << "-----------------------" << endl ;
if (star.is_irrotational()) {
ost << "irrotational configuration" << endl ;
}
else {
ost << "corotating configuration" << endl ;
}
ost << "Absolute abscidia of the stellar center: "
<< star.get_mp().get_ori_x()/km << " km" << endl ;
ost << "Orientation with respect to the absolute frame : "
<< star.get_mp().get_rot_phi() << " rad" << endl ;
double r0 = 0.5 * ( star.ray_eq() + star.ray_eq_pi() ) ;
// = 1 in Baumgarte et al.
double d_ns = separ + star.ray_eq() - r0 ;
// Orbital separation of Baumgarte et al.
double d_tilde = d_ns / r0 ; // Normalized separation of Baumgarte et al.
ost << endl << "Comparison with those by Baumgarte et al. :" << endl ;
ost << " Radius r0 : " << r0 / km << " km " << endl ;
ost << " Separation d : " << d_ns / km << " km " << endl ;
ost << " Normalized sep. (d/r0) : " << d_tilde << endl ;
ost << endl << "Black hole : " ;
ost << endl << "========== " << endl ;
ost << "Gravitational mass of BH : "
<< mass_bh / msol << " M_sol" << endl ;
return ost ;
}
// Display in polytropic units
// ---------------------------
void Bin_bhns_extr::display_poly(ostream& ost) const {
using namespace Unites ;
const Eos* p_eos = &( star.get_eos() ) ;
const Eos_poly* p_eos_poly = dynamic_cast<const Eos_poly*>( p_eos ) ;
if (p_eos_poly != 0x0) {
double kappa = p_eos_poly->get_kap() ;
double gamma = p_eos_poly->get_gam() ;
double kap_ns2 = pow( kappa, 0.5 /(gamma-1) ) ;
// Polytropic unit of length in terms of r_unit :
double r_poly = kap_ns2 / sqrt(ggrav) ;
// Polytropic unit of time in terms of t_unit :
double t_poly = r_poly ;
// Polytropic unit of mass in terms of m_unit :
double m_poly = r_poly / ggrav ;
// Polytropic unit of angular momentum in terms of j_unit :
// double j_poly = r_poly * r_poly / ggrav ;
double r0 = 0.5 * ( star.ray_eq() + star.ray_eq_pi() ) ;
// = 1 in Baumgarte et al.
double d_ns = separ + star.ray_eq() - r0 ;
// Orbital separation of Baumgarte et al.
ost.precision(16) ;
ost << endl << "Quantities in polytropic units : " ;
ost << endl << "==============================" << endl ;
ost << " ( r_poly = " << r_poly / km << " km )" << endl ;
ost << " d_e_max : " << separ / r_poly << endl ;
ost << " d_G_x : " << xa_barycenter_extr() / r_poly << endl
<< " d_G_y : " << ya_barycenter_extr() / r_poly << endl ;
ost << " d_bh/M_bh : " << d_ns/r_poly / (mass_bh/m_poly) << endl ;
ost << " Omega : " << omega * t_poly << endl ;
ost << " Omega M_bh : " << omega * t_poly * mass_bh / m_poly
<< endl ;
ost << " M_bar(NS) : " << mass_b_extr() / m_poly << endl ;
ost << " M_bar(NS_0) : " << star.mass_b() / m_poly << endl ;
ost << " R_0(NS) : "
<< 0.5 * (star.ray_eq() + star.ray_eq_pi()) / r_poly << endl ;
ost << " M_grv(BH) : " << mass_bh / m_poly << endl ;
}
}
}
|
