/usr/include/lorene/C++/Include/binary.h is in liblorene-dev 0.0.0~cvs20161116+dfsg-1.
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* Definition of Lorene class Binary
*
*/
/*
* Copyright (c) 2004 Limousin Francois
*
* 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
*
*/
#ifndef __BINARY_H_
#define __BINARY_H_
/*
* $Id: binary.h,v 1.10 2014/10/13 08:52:32 j_novak Exp $
* $Log: binary.h,v $
* Revision 1.10 2014/10/13 08:52:32 j_novak
* Lorene classes and functions now belong to the namespace Lorene.
*
* Revision 1.9 2006/04/11 14:26:12 f_limousin
* New version of the code : improvement of the computation of some
* critical sources, estimation of the dirac gauge, helical symmetry...
*
* Revision 1.8 2005/11/08 20:17:55 f_limousin
* Add function dirac_gauge() used to impose Dirac gauge during an iteration.
*
* Revision 1.7 2005/09/15 15:56:28 e_gourgoulhon
* Made the documentation compliant with Doxygen.
*
* Revision 1.6 2005/09/13 19:38:32 f_limousin
* Reintroduction of the resolution of the equations in cartesian coordinates.
*
* Revision 1.5 2004/07/21 11:45:20 f_limousin
* Add function mass_adm_vol() to compute the ADM mass of the system
* with a volume integral instead of a surface one.
*
* Revision 1.4 2004/05/25 14:50:06 f_limousin
* Add the virial theorem for conformally flat configurations.
*
* Revision 1.3 2004/01/20 15:25:39 f_limousin
* Nex class binary
*
*
* $Header: /cvsroot/Lorene/C++/Include/binary.h,v 1.10 2014/10/13 08:52:32 j_novak Exp $
*
*/
// Lorene headers
#include "star.h"
namespace Lorene {
/**
* Binary systems. *** UNDER DEVELOPMENT *** \ingroup (star)
*
* @version #$Id: binary.h,v 1.10 2014/10/13 08:52:32 j_novak Exp $#
*/
class Binary {
// Data :
// -----
protected:
/// First star of the system
Star_bin star1 ;
/// Second star of the system
Star_bin star2 ;
/** Array of the two stars (to perform loops on the stars):
* \c et[0] contains the address of \c star1 and \c et[1]
* that of \c star2.
*/
Star_bin* et[2] ;
/** Angular velocity with respect to an asymptotically inertial
* observer
*/
double omega ;
/** Absolute X coordinate of the rotation axis
*/
double x_axe ;
// Derived data :
// ------------
protected:
/// Total ADM mass of the system
mutable double* p_mass_adm ;
/// Total Komar mass of the system
mutable double* p_mass_kom ;
/// Total angular momentum of the system
mutable Tbl* p_angu_mom ;
/// Total energy of the system
mutable double* p_total_ener ;
/// Virial theorem error
mutable double* p_virial ;
/// Relative error on the Hamiltonian constraint
mutable double* p_ham_constr ;
/// Relative error on the momentum constraint
mutable Tbl* p_mom_constr ;
// Constructors - Destructor
// -------------------------
public:
/** Standard constructor.
*
* @param mp1 Mapping on which \c star1 will be defined
* @param nzet1 Number of domains occupied by \c star1
* @param eos1 Equation of state of \c star1
* @param irrot1 should be \c true if \c star1 is irrotational,
* \c false if \c star1 is corotating
* @param mp2 Mapping on which \c star2 will be defined
* @param nzet2 Number of domains occupied by \c star2
* @param eos2 Equation of state of \c star2
* @param irrot2 should be \c true if \c star2 is irrotational,
* \c false if \c star2 is corotating
* @param conf_flat should be \c true for a 3-metric conformally
* flat and \c false for a more general one.
*/
Binary(Map& mp1, int nzet1, const Eos& eos1, int irrot1,
Map& mp2, int nzet2, const Eos& eos2, int irrot2,
int conf_flat) ;
Binary(const Binary& ) ; ///< Copy constructor
/** Constructor from a file (see \c sauve(FILE* )).
*
* @param mp1 Mapping on which \c star1 will be defined
* @param eos1 Equation of state of \c star1
* @param mp2 Mapping on which \c star2 will be defined
* @param eos2 Equation of state of \c star2
* @param fich input file (must have been created by the function
* \c sauve)
*/
Binary(Map& mp1, const Eos& eos1, Map& mp2, const Eos& eos2,
FILE* fich) ;
~Binary() ; ///< Destructor
// Memory management
// -----------------
protected:
/// Deletes all the derived quantities
void del_deriv() const ;
/// Sets to \c 0x0 all the pointers on derived quantities
void set_der_0x0() const ;
// Mutators / assignment
// ---------------------
public:
/// Assignment to another \c Binary
void operator=(const Binary&) ;
/// Read/write of the star no. i
Star_bin& set(int i)
{ assert( (i==1) || (i==2) );
del_deriv() ;
return *et[i-1] ;} ;
/// Sets the orbital angular velocity [\c f_unit]
double& set_omega() {return omega; } ;
/// Sets the absolute coordinate X of the rotation axis [\c r_unit]
double& set_x_axe() {return x_axe; } ;
// Accessors
// ---------
public:
/// Returns a reference to the star no. i
const Star_bin& operator()(int i) const
{ assert( (i==1) || (i==2) );
return *et[i-1] ;} ;
/// Returns the orbital angular velocity [\c f_unit]
double get_omega() const {return omega; } ;
/// Returns the absolute coordinate X of the rotation axis [\c r_unit]
double get_x_axe() const {return x_axe; } ;
/** Returns the coordinate separation of the two stellar
* centers [\c r_unit]
*/
double separation() const ;
// Outputs
// -------
public:
void sauve(FILE *) const ; ///< Save in a file
/// Display
friend ostream& operator<<(ostream& , const Binary& ) ;
/// Display in polytropic units
void display_poly(ostream& ) const ;
/** Write global quantities in a formatted file.
* This file can be read by an external program.
*/
void write_global(ostream& ) const ;
private:
/// Operator >> (function called by the operator <<).
ostream& operator>>(ostream& ) const ;
// Computational routines
// ----------------------
public:
/// Total ADM mass
double mass_adm() const ;
/// Total ADM mass (computed by a volume integral)
double mass_adm_vol() const ;
/// Total Komar mass
double mass_kom() const ;
/// Total Komar mass (computed by a volume integral)
double mass_kom_vol() const ;
/** Total angular momentum.
*
* @return 1-D \c Tbl of size 3, according to
* \li \c angu_mom()(0) = \f$J^r\f$,
* \li \c angu_mom()(1) = \f$J^t\f$,
* \li \c angu_mom()(2) = \f$J^p\f$.
*/
const Tbl& angu_mom() const ;
/** Total energy (excluding the rest mass energy).
*
* In the Newtonian case, it is defined as the sum of kinetic,
* internal, and gravitational potential energies.
*
* In the relativistic case, it is defined as
* \f$M_{\rm ADM} - M_{\rm bar,1} - M_{\rm bar,2}\f$.
*/
double total_ener() const ;
/** Estimates the relative error on the virial theorem
*/
double virial() const ;
/** Estimates the relative error on the Hamiltonian constraint
*/
double ham_constr() const ;
/** Estimates the relative error on the momentum constraint
*/
const Tbl& mom_constr() const ;
/** Computes the orbital angular velocity \c omega and the
* position of the rotation axis \c x_axe.
*
* @param fact_omeg_min [input] : determines the lower bound of the
* interval \c [omega_min, omega_max] in which
* \c omega is searched by
* \c omega_min = fact_omeg_min * omega,
* where \c omega is the previous value of the
* angular velocity
* (typical value : \c fact_omeg_min = 0.5)
*
* @param fact_omeg_max [input] : determines the higher bound of the
* interval \c [omega_min, omega_max] in which
* \c omega is searched by
* \c omega_max = fact_omeg_max * omega,
* where \c omega is the previous value of the
* angular velocity.
* (typical value : \c fact_omeg_max = 1.5)
*
* @param xgg1 [output] : x coordinate (relative to star 1 mapping)
* of the ``center of mass'' of star 1
*
* @param xgg2 [output] : x coordinate (relative to star 2 mapping)
* of the ``center of mass'' of star 2
*
*/
void orbit(double fact_omeg_min, double fact_omeg_max, double& xgg1,
double& xgg2) ;
/** Sets the orbital angular velocity to some 2-PN analytical
* value (Keplerian value in the Newtonian case)
*/
void analytical_omega() ;
/** Sets some analytical template for the shift vector (via the
* members \c w_shift and \c khi_shift of the two
* \c Star_bin.
*/
void analytical_shift() ;
/**
* Calculates \c decouple which is used to obtain
* \c qq_auto by the formula :
* \c qq_auto = \c decouple * \c qq.
* (see the membre \c Scalar \c decouple for more
* precisions about its value).
*
*/
void fait_decouple () ;
/// Function used to impose Dirac gauge during an iteration
void dirac_gauge() ;
/// Function testing the helical symmetry
void helical() ;
};
ostream& operator<<(ostream& , const Binary& ) ;
}
#endif
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