Extended description of the class for Doc++ documentation. More...
#include <bin_ns_ncp.h>
Public Member Functions | |
| Bin_ns_ncp (Map &mp1, int nzet1, const Eos &eos1, int irrot1, Map &mp2, int nzet2, const Eos &eos2, int irrot2, int relat, int conf_flat, const Metrique &flat1, const Metrique &flat2, const Tenseur_sym &source1, const Tenseur_sym &source2) | |
| Standard constructor. | |
| Bin_ns_ncp (const Bin_ns_ncp &) | |
| Bin_ns_ncp (Map &mp1, const Eos &eos1, Map &mp2, const Eos &eos2, const Metrique &flat1, const Metrique &flat2, FILE *fich) | |
| Copy constructor. | |
| void | operator= (const Bin_ns_ncp &) |
| Assignment to another { Bin_ns_ncp}. | |
| Et_bin_ncp & | set (int i) |
| Read/write of the star no. i. | |
| double & | set_omega () |
| Sets the orbital angular velocity [{ f}]. | |
| double & | set_x_axe () |
| Sets the absolute coordinate X of the rotation axis [{ r}]. | |
| const Et_bin_ncp & | operator() (int i) const |
| Returns a reference to the star no. i. | |
| double | get_omega () const |
| Returns the orbital angular velocity [{ f}]. | |
| double | get_x_axe () const |
| Returns the absolute coordinate X of the rotation axis [{ r}]. | |
| double | separation () const |
| Returns the coordinate separation of the two stellar centers [{ r}]. | |
| void | sauve (FILE *) const |
| void | display_poly (ostream &) const |
| Display in polytropic units. | |
| void | write_global (ostream &) const |
| Write global quantities in a formatted file. | |
| double | mass_adm () const |
| Total ADM mass. | |
| double | mass_kom () const |
| Total Komar mass. | |
| const Tbl & | angu_mom () const |
| Total angular momentum. | |
| double | total_ener () const |
| Total energy (excluding the rest mass energy). | |
| double | virial () const |
| Estimates the relative error on the virial theorem (for a relativistic one, it returns $|1 - M_{ Komar} / M_{ ADM}|$). | |
| double | virial_gb () const |
| Estimates the relative error on the virial theorem calculated by E.Gourgoulhon and S.Bonazzola (Class. | |
| double | virial_fus () const |
| Estimates the relative error on the virial theorem calculated by J.L.Friedman, K.Uryu, and M.Shibata (PRD accepted, gr-qc/0108070). | |
| double | ham_constr () const |
| Estimates the relative error on the Hamiltonian constraint equation by comparing $ A$ with {equation} -4 A^2 E - {A^2 4} K_{ij} K^{ij} - {1 2} {}_i A {}^i A {equation}. | |
| const Tbl & | mom_constr () const |
| Estimates the relative error on the momentum constraint equation by comparing ${}_j K^{ij}$ with {equation} 8 J^i - 5 K^{ij} {}_j A {equation}. | |
| void | orbit (double fact_omeg_min, double fact_omeg_max, double &xgg1, double &xgg2) |
| Computes the orbital angular velocity { omega} and the position of the rotation axis { x}. | |
| void | analytical_omega () |
| Sets the orbital angular velocity to some 2-PN analytical value (Keplerian value in the Newtonian case). | |
| void | analytical_shift () |
| Sets some analytical template for the shift vector (via the members { w} and { khi} of the two { Etoile}. | |
| void | compare (FILE *) |
| Performs a comparison between quantities as the shift, lapse and tkij_auto for two two binaries stars. | |
| void | compare (const Binaire &) |
| Performs a comparison between quantities as the shift, lapse and tkij_auto for two two binaries stars. | |
| void | fait_decouple () |
| Calculates {tt decouple} which is used to obtain { a_car} by the formula : { a_car} = { decouple} * { a_car}. | |
Protected Member Functions | |
| void | del_deriv () const |
| Destructor. | |
| void | set_der_0x0 () const |
| Sets to { 0x0} all the pointers on derived quantities. | |
Protected Attributes | |
| Et_bin_ncp | star1 |
| First star ncp of the system. | |
| Et_bin_ncp | star2 |
| Second star ncp of the system. | |
| Et_bin_ncp * | et [2] |
| Array of the two stars (to perform loops on the stars): { et[0]} contains the address of { star1} and { et[1]} that of { star2}. | |
| double | omega |
| Angular velocity with respect to an asymptotically inertial observer. | |
| double | x_axe |
| Absolute X coordinate of the rotation axis. | |
| double * | p_mass_adm |
| Total ADM mass of the system. | |
| double * | p_mass_kom |
| Total Komar mass of the system. | |
| Tbl * | p_angu_mom |
| Total angular momentum of the system. | |
| double * | p_total_ener |
| Total energy of the system. | |
| double * | p_virial |
| Virial theorem error. | |
| double * | p_virial_gb |
| Virial theorem error by E.Gourgoulhon and S.Bonazzola. | |
| double * | p_virial_fus |
| Virial theorem error by J.L.Friedman, K.Uryu, and M.Shibata. | |
| double * | p_ham_constr |
| Relative error on the Hamiltonian constraint. | |
| Tbl * | p_mom_constr |
| Relative error on the momentum constraint. | |
Private Member Functions | |
| ostream & | operator>> (ostream &) const |
| Operator >> (function called by the operator <<). | |
Friends | |
| ostream & | operator<< (ostream &, const Bin_ns_ncp &) |
| Save in a file. | |
Extended description of the class for Doc++ documentation.
Definition at line 66 of file bin_ns_ncp.h.
| Bin_ns_ncp::Bin_ns_ncp | ( | Map & | mp1, | |
| int | nzet1, | |||
| const Eos & | eos1, | |||
| int | irrot1, | |||
| Map & | mp2, | |||
| int | nzet2, | |||
| const Eos & | eos2, | |||
| int | irrot2, | |||
| int | relat, | |||
| int | conf_flat, | |||
| const Metrique & | flat1, | |||
| const Metrique & | flat2, | |||
| const Tenseur_sym & | source1, | |||
| const Tenseur_sym & | source2 | |||
| ) |
Standard constructor.
| mp1 | Mapping on which { star1} will be defined | |
| nzet1 | Number of domains occupied by { star1} | |
| eos1 | Equation of state of { star1} | |
| irrot1 | should be { true} if { star1} is irrotational, { false} if { star1} is corotating | |
| mp2 | Mapping on which { star2} will be defined | |
| nzet2 | Number of domains occupied by { star2} | |
| eos2 | Equation of state of { star2} | |
| irrot2 | should be { true} if { star2} is irrotational, { false} if { star2} is corotating | |
| relat | should be { true} for a relativistic configuration, { false} for a Newtonian one |
| Bin_ns_ncp::Bin_ns_ncp | ( | Map & | mp1, | |
| const Eos & | eos1, | |||
| Map & | mp2, | |||
| const Eos & | eos2, | |||
| const Metrique & | flat1, | |||
| const Metrique & | flat2, | |||
| FILE * | fich | |||
| ) |
Copy constructor.
Constructor from a file (see { sauve(FILE* )}).
| mp1 | Mapping on which { star1} will be defined | |
| eos1 | Equation of state of { star1} | |
| mp2 | Mapping on which { star2} will be defined | |
| eos2 | Equation of state of { star2} | |
| fich | input file (must have been created by the function { sauve}) |
| void Bin_ns_ncp::analytical_omega | ( | ) |
Sets the orbital angular velocity to some 2-PN analytical value (Keplerian value in the Newtonian case).
| void Bin_ns_ncp::analytical_shift | ( | ) |
Sets some analytical template for the shift vector (via the members { w} and { khi} of the two { Etoile}.
| const Tbl& Bin_ns_ncp::angu_mom | ( | ) | const |
Total angular momentum.
| void Bin_ns_ncp::compare | ( | const Binaire & | ) |
Performs a comparison between quantities as the shift, lapse and tkij_auto for two two binaries stars.
| void Bin_ns_ncp::compare | ( | FILE * | ) |
Performs a comparison between quantities as the shift, lapse and tkij_auto for two two binaries stars.
This method takes a fich as argument to construct the etoile_bin.
| void Bin_ns_ncp::del_deriv | ( | ) | const [protected] |
Destructor.
Deletes all the derived quantities
| void Bin_ns_ncp::display_poly | ( | ostream & | ) | const |
Display in polytropic units.
| void Bin_ns_ncp::fait_decouple | ( | ) |
Calculates {tt decouple} which is used to obtain { a_car} by the formula : { a_car} = { decouple} * { a_car}.
(see the membre {tt Cmp decouple} for more precisions about its value).
| double Bin_ns_ncp::get_omega | ( | ) | const [inline] |
Returns the orbital angular velocity [{ f}].
Definition at line 208 of file bin_ns_ncp.h.
References omega.
| double Bin_ns_ncp::get_x_axe | ( | ) | const [inline] |
Returns the absolute coordinate X of the rotation axis [{ r}].
Definition at line 211 of file bin_ns_ncp.h.
References x_axe.
| double Bin_ns_ncp::ham_constr | ( | ) | const |
Estimates the relative error on the Hamiltonian constraint equation by comparing $ A$ with {equation} -4 A^2 E - {A^2 4} K_{ij} K^{ij} - {1 2} {}_i A {}^i A {equation}.
| double Bin_ns_ncp::mass_adm | ( | ) | const |
Total ADM mass.
| double Bin_ns_ncp::mass_kom | ( | ) | const |
Total Komar mass.
| const Tbl& Bin_ns_ncp::mom_constr | ( | ) | const |
Estimates the relative error on the momentum constraint equation by comparing ${}_j K^{ij}$ with {equation} 8 J^i - 5 K^{ij} {}_j A {equation}.
| const Et_bin_ncp& Bin_ns_ncp::operator() | ( | int | i | ) | const [inline] |
| void Bin_ns_ncp::operator= | ( | const Bin_ns_ncp & | ) |
Assignment to another { Bin_ns_ncp}.
| ostream& Bin_ns_ncp::operator>> | ( | ostream & | ) | const [private] |
Operator >> (function called by the operator <<).
| void Bin_ns_ncp::orbit | ( | double | fact_omeg_min, | |
| double | fact_omeg_max, | |||
| double & | xgg1, | |||
| double & | xgg2 | |||
| ) |
Computes the orbital angular velocity { omega} and the position of the rotation axis { x}.
| fact_omeg_min | [input] : determines the lower bound of the interval { [omega, omega]} in which { omega} is searched by { omega = fact * omega}, where { omega} is the previous value of the angular velocity (typical value : { fact = 0.5}) | |
| fact_omeg_max | [input] : determines the higher bound of the interval { [omega, omega]} in which { omega} is searched by { omega = fact * omega}, where { omega} is the previous value of the angular velocity. (typical value : { fact = 1.5}) | |
| xgg1 | [output] : x coordinate (relative to star 1 mapping) of the ``center of mass'' of star 1 | |
| xgg2 | [output] : x coordinate (relative to star 2 mapping) of the ``center of mass'' of star 2 |
| double Bin_ns_ncp::separation | ( | ) | const |
Returns the coordinate separation of the two stellar centers [{ r}].
| Et_bin_ncp& Bin_ns_ncp::set | ( | int | i | ) | [inline] |
Read/write of the star no. i.
Definition at line 187 of file bin_ns_ncp.h.
References del_deriv(), and et.
| void Bin_ns_ncp::set_der_0x0 | ( | ) | const [protected] |
Sets to { 0x0} all the pointers on derived quantities.
| double& Bin_ns_ncp::set_omega | ( | ) | [inline] |
Sets the orbital angular velocity [{ f}].
Definition at line 193 of file bin_ns_ncp.h.
References omega.
| double& Bin_ns_ncp::set_x_axe | ( | ) | [inline] |
Sets the absolute coordinate X of the rotation axis [{ r}].
Definition at line 196 of file bin_ns_ncp.h.
References x_axe.
| double Bin_ns_ncp::total_ener | ( | ) | 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 $M_{ ADM} - M_{ bar,1} - M_{ bar,2}$.
| double Bin_ns_ncp::virial | ( | ) | const |
Estimates the relative error on the virial theorem (for a relativistic one, it returns $|1 - M_{ Komar} / M_{ ADM}|$).
| double Bin_ns_ncp::virial_fus | ( | ) | const |
Estimates the relative error on the virial theorem calculated by J.L.Friedman, K.Uryu, and M.Shibata (PRD accepted, gr-qc/0108070).
The expression used in the LORENE is Eq.(5.7) in the paper by M.Shibata and K.Uryu (PRD64, 104017 (2001))
| double Bin_ns_ncp::virial_gb | ( | ) | const |
Estimates the relative error on the virial theorem calculated by E.Gourgoulhon and S.Bonazzola (Class.
Quantum Grav. 11, 443 (1994): Eq.(29)) normalized by $2 G$.
| void Bin_ns_ncp::write_global | ( | ostream & | ) | const |
Write global quantities in a formatted file.
This file can be read by an external program.
| ostream& operator<< | ( | ostream & | , | |
| const Bin_ns_ncp & | ||||
| ) | [friend] |
Save in a file.
Display
Et_bin_ncp* Bin_ns_ncp::et[2] [protected] |
Array of the two stars (to perform loops on the stars): { et[0]} contains the address of { star1} and { et[1]} that of { star2}.
Definition at line 82 of file bin_ns_ncp.h.
double Bin_ns_ncp::omega [protected] |
Angular velocity with respect to an asymptotically inertial observer.
Definition at line 87 of file bin_ns_ncp.h.
Tbl* Bin_ns_ncp::p_angu_mom [mutable, protected] |
Total angular momentum of the system.
Definition at line 104 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_ham_constr [mutable, protected] |
Relative error on the Hamiltonian constraint.
Definition at line 119 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_mass_adm [mutable, protected] |
Total ADM mass of the system.
Definition at line 98 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_mass_kom [mutable, protected] |
Total Komar mass of the system.
Definition at line 101 of file bin_ns_ncp.h.
Tbl* Bin_ns_ncp::p_mom_constr [mutable, protected] |
Relative error on the momentum constraint.
Definition at line 122 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_total_ener [mutable, protected] |
Total energy of the system.
Definition at line 107 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_virial [mutable, protected] |
Virial theorem error.
Definition at line 110 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_virial_fus [mutable, protected] |
Virial theorem error by J.L.Friedman, K.Uryu, and M.Shibata.
Definition at line 116 of file bin_ns_ncp.h.
double* Bin_ns_ncp::p_virial_gb [mutable, protected] |
Virial theorem error by E.Gourgoulhon and S.Bonazzola.
Definition at line 113 of file bin_ns_ncp.h.
Et_bin_ncp Bin_ns_ncp::star1 [protected] |
First star ncp of the system.
Definition at line 73 of file bin_ns_ncp.h.
Et_bin_ncp Bin_ns_ncp::star2 [protected] |
Second star ncp of the system.
Definition at line 76 of file bin_ns_ncp.h.
double Bin_ns_ncp::x_axe [protected] |
Absolute X coordinate of the rotation axis.
Definition at line 91 of file bin_ns_ncp.h.
1.6.1