Class for differentially rotating stars in quasi-isotropic gauge and maximal slicing. More...

#include <star_rot_diff.h>

Inheritance diagram for Lorene::Star_rot_diff:

Public Member Functions
	Star_rot_diff (Map &mp_i, int nzet_i, bool relat, const Eos &eos_i, double(omega_frot_i)(double, const Tbl &), double(primfrot_i)(double, const Tbl &), const Tbl &par_frot_i)
	Standard constructor. More...

	Star_rot_diff (const Star_rot_diff &)
	Copy constructor. More...

	Star_rot_diff (Map &mp_i, const Eos &eos_i, FILE fich, double(omega_frot_i)(double, const Tbl &), double(*primfrot_i)(double, const Tbl &))
	Constructor from a file (see `sauve(FILE*)` ). More...

virtual	~Star_rot_diff ()
	Destructor. More...

void	operator= (const Star_rot_diff &)
	Assignment to another `Star_rot_diff`. More...

const Scalar &	get_omega_field () const
	Returns the angular velocity field $\Omega$ . More...

virtual double	get_omega_c () const
	Returns the central value of the rotation angular velocity ([f_unit] ) More...

virtual void	sauve (FILE *) const
	Save in a file. More...

virtual void	display_poly (ostream &) const
	Display in polytropic units. More...

virtual double	tsw () const
	Ratio T/W. More...

virtual void	hydro_euler ()
	Computes the hydrodynamical quantities relative to the Eulerian observer from those in the fluid frame. More...

void	fait_omega_field (double omeg_min, double omeg_max, double precis, int nitermax)
	Computes $\Omega(r,\theta)$ (member `omega_field` ). More...

void	fait_prim_field ()
	Computes the member `prim_field` from `omega_field` . More...

double	omega_funct (double F) const
	Evaluates $\Omega(F)$ , where F is linked to the components of the fluid 4-velocity by $F = u^t u_\varphi \ .$ . More...

double	prim_funct_omega (double F) const
	Evaluates the primitive of $F\frac{d\Omega(F)}{dF}$ . More...

virtual void	equilibrium (double ent_c, double omega0, double fact_omega, int nzadapt, const Tbl &ent_limit, const Itbl &icontrol, const Tbl &control, double mbar_wanted, double aexp_mass, Tbl &diff, Param *=0x0)
	Computes an equilibrium configuration. More...

bool	is_relativistic () const
	Returns `true` for a relativistic star, `false` for a Newtonian one. More...

const Scalar &	get_bbb () const
	Returns the metric factor B. More...

const Scalar &	get_a_car () const
	Returns the square of the metric factor A. More...

const Scalar &	get_b_car () const
	Returns the square of the metric factor B. More...

const Scalar &	get_nphi () const
	Returns the metric coefficient $N^\varphi$ . More...

const Scalar &	get_tnphi () const
	Returns the component $\tilde N^\varphi = N^\varphi r\sin\theta$ of the shift vector. More...

const Scalar &	get_uuu () const
	Returns the norm of `u_euler`. More...

const Scalar &	get_nuf () const
	Returns the part of the Metric potential $\nu = \ln N$ = `logn` generated by the matter terms. More...

const Scalar &	get_nuq () const
	Returns the Part of the Metric potential $\nu = \ln N$ = `logn` generated by the quadratic terms. More...

const Scalar &	get_dzeta () const
	Returns the Metric potential $\zeta = \ln(AN)$ . More...

const Scalar &	get_tggg () const
	Returns the Metric potential $\tilde G = (NB-1) r\sin\theta$ . More...

const Vector &	get_w_shift () const
	Returns the vector used in the decomposition of `shift` , following Shibata's prescription [Prog. More...

const Scalar &	get_khi_shift () const
	Returns the scalar $\chi$ used in the decomposition of `shift` following Shibata's prescription [Prog. More...

const Sym_tensor &	get_tkij () const
	Returns the tensor ${\tilde K_{ij}}$ related to the extrinsic curvature tensor by ${\tilde K_{ij}} = B^{-2} K_{ij}$ . More...

const Scalar &	get_ak_car () const
	Returns the scalar $A^2 K_{ij} K^{ij}$ . More...

virtual const Itbl &	l_surf () const
	Description of the stellar surface: returns a 2-D `Itbl` containing the values of the domain index l on the surface at the collocation points in $(\theta', \phi')$ . More...

virtual double	mass_b () const
	Baryon mass. More...

virtual double	mass_g () const
	Gravitational mass. More...

virtual double	angu_mom () const
	Angular momentum. More...

virtual double	grv2 () const
	Error on the virial identity GRV2. More...

virtual double	grv3 (ostream *ost=0x0) const
	Error on the virial identity GRV3. More...

virtual double	r_circ () const
	Circumferential equatorial radius. More...

virtual double	r_circ_merid () const
	Crcumferential meridional radius. More...

virtual double	aplat () const
	Flatening r_pole/r_eq. More...

virtual double	area () const
	Integrated surface area in ${\rm km}^2$ . More...

virtual double	mean_radius () const
	Mean star radius from the area $r_{\rm mean} = \sqrt{\mathcal{A}} / 4\pi$ . More...

virtual double	z_eqf () const
	Forward redshift factor at equator. More...

virtual double	z_eqb () const
	Backward redshift factor at equator. More...

virtual double	z_pole () const
	Redshift factor at North pole. More...

virtual double	mom_quad () const
	Quadrupole moment. More...

virtual const Tbl &	surf_grav () const
	Surface gravity (table along the theta direction) More...

virtual double	r_isco (ostream *ost=0x0) const
	Circumferential radius of the innermost stable circular orbit (ISCO). More...

virtual double	f_isco () const
	Orbital frequency at the innermost stable circular orbit (ISCO). More...

virtual double	espec_isco () const
	Energy of a particle on the ISCO. More...

virtual double	lspec_isco () const
	Angular momentum of a particle on the ISCO. More...

virtual double	f_eq () const
	Orbital frequency at the equator. More...

void	update_metric ()
	Computes metric coefficients from known potentials. More...

void	fait_shift ()
	Computes `shift` from `w_shift` and `khi_shift` according to Shibata's prescription [Prog. More...

void	fait_nphi ()
	Computes `tnphi` and `nphi` from the Cartesian components of the shift, stored in `shift` . More...

void	extrinsic_curvature ()
	Computes `tkij` and `ak_car` from `shift` , `nnn` and `b_car` . More...

Map &	set_mp ()
	Read/write of the mapping. More...

void	set_enthalpy (const Scalar &)
	Assignment of the enthalpy field. More...

void	equation_of_state ()
	Computes the proper baryon and energy density, as well as pressure from the enthalpy. More...

virtual void	equilibrium_spher (double ent_c, double precis=1.e-14, const Tbl *pent_limit=0x0)
	Computes a spherical static configuration. More...

const Map &	get_mp () const
	Returns the mapping. More...

int	get_nzet () const
	Returns the number of domains occupied by the star. More...

const Eos &	get_eos () const
	Returns the equation of state. More...

const Scalar &	get_ent () const
	Returns the enthalpy field. More...

const Scalar &	get_nbar () const
	Returns the proper baryon density. More...

const Scalar &	get_ener () const
	Returns the proper total energy density. More...

const Scalar &	get_press () const
	Returns the fluid pressure. More...

const Scalar &	get_ener_euler () const
	Returns the total energy density with respect to the Eulerian observer. More...

const Scalar &	get_s_euler () const
	Returns the trace of the stress tensor in the Eulerian frame. More...

const Scalar &	get_gam_euler () const
	Returns the Lorentz factor between the fluid and Eulerian observers. More...

const Vector &	get_u_euler () const
	Returns the fluid 3-velocity with respect to the Eulerian observer. More...

const Tensor &	get_stress_euler () const
	Returns the spatial part of the stress-energy tensor with respect to the Eulerian observer. More...

const Scalar &	get_logn () const
	Returns the logarithm of the lapse N. More...

const Scalar &	get_nn () const
	Returns the lapse function N. More...

const Vector &	get_beta () const
	Returns the shift vector $\beta^i$ . More...

const Scalar &	get_lnq () const

const Metric &	get_gamma () const
	Returns the 3-metric $\gamma$ . More...

double	ray_eq () const
	Coordinate radius at $\phi=0$ , $\theta=\pi/2$ [r_unit]. More...

double	ray_eq_pis2 () const
	Coordinate radius at $\phi=\pi/2$ , $\theta=\pi/2$ [r_unit]. More...

double	ray_eq_pi () const
	Coordinate radius at $\phi=\pi$ , $\theta=\pi/2$ [r_unit]. More...

double	ray_eq_3pis2 () const
	Coordinate radius at $\phi=3\pi/2$ , $\theta=\pi/2$ [r_unit]. More...

double	ray_pole () const
	Coordinate radius at $\theta=0$ [r_unit]. More...

const Tbl &	xi_surf () const
	Description of the stellar surface: returns a 2-D `Tbl` containing the values of the radial coordinate $\xi$ on the surface at the collocation points in $(\theta', \phi')$ . More...

Static Public Member Functions
static double	lambda_grv2 (const Scalar &sou_m, const Scalar &sou_q)
	Computes the coefficient $\lambda$ which ensures that the GRV2 virial identity is satisfied. More...

Protected Member Functions
virtual ostream &	operator>> (ostream &) const
	Operator >> (virtual function called by the operator <<). More...

virtual void	del_deriv () const
	Deletes all the derived quantities. More...

virtual void	set_der_0x0 () const
	Sets to `0x0` all the pointers on derived quantities. More...

virtual void	del_hydro_euler ()
	Sets to `ETATNONDEF` (undefined state) the hydrodynamical quantities relative to the Eulerian observer. More...

virtual void	partial_display (ostream &) const
	Printing of some informations, excluding all global quantities. More...

Protected Attributes
double(*	omega_frot )(double, const Tbl &)
	Function $\Omega(F)$ defining the rotation profile. More...

double(*	primfrot )(double, const Tbl &)
	Primitive of the function $F\frac{d\Omega(F)}{dF}$ , which vanishes at the stellar center. More...

Tbl	par_frot
	Parameters of the function $\Omega(F)$ . More...

Scalar	omega_field
	Field $\Omega(r,\theta)$ . More...

double	omega_min
	Minimum value of $\Omega$ . More...

double	omega_max
	Maximum value of $\Omega$ . More...

Scalar	prim_field
	Field $\int_0^F F'\,\frac{d\Omega(F')}{dF'} \, dF'$ . More...

bool	relativistic
	Indicator of relativity: `true` for a relativistic star, `false` for a Newtonian one. More...

double	unsurc2
	: `unsurc2=1` for a relativistic star, 0 for a Newtonian one. More...

double	omega
	Rotation angular velocity ([f_unit] ) More...

Scalar	a_car
	Square of the metric factor A. More...

Scalar	bbb
	Metric factor B. More...

Scalar	b_car
	Square of the metric factor B. More...

Scalar	nphi
	Metric coefficient $N^\varphi$ . More...

Scalar	tnphi
	Component $\tilde N^\varphi = N^\varphi r\sin\theta$ of the shift vector. More...

Scalar	uuu
	Norm of `u_euler`. More...

Scalar	nuf
	Part of the Metric potential $\nu = \ln N$ = `logn` generated by the matter terms. More...

Scalar	nuq
	Part of the Metric potential $\nu = \ln N$ = `logn` generated by the quadratic terms. More...

Scalar	dzeta
	Metric potential $\zeta = \ln(AN)$ . More...

Scalar	tggg
	Metric potential $\tilde G = (NB-1) r\sin\theta$ . More...

Vector	w_shift
	Vector used in the decomposition of `shift` , following Shibata's prescription [Prog. More...

Scalar	khi_shift
	Scalar $\chi$ used in the decomposition of `shift` , following Shibata's prescription [Prog. More...

Sym_tensor	tkij
	Tensor ${\tilde K_{ij}}$ related to the extrinsic curvature tensor by ${\tilde K_{ij}} = B^{-2} K_{ij}$ . More...

Scalar	ak_car
	Scalar $A^2 K_{ij} K^{ij}$ . More...

Scalar	ssjm1_nuf
	Effective source at the previous step for the resolution of the Poisson equation for `nuf` by means of `Map_et::poisson` . More...

Scalar	ssjm1_nuq
	Effective source at the previous step for the resolution of the Poisson equation for `nuq` by means of `Map_et::poisson` . More...

Scalar	ssjm1_dzeta
	Effective source at the previous step for the resolution of the Poisson equation for `dzeta` . More...

Scalar	ssjm1_tggg
	Effective source at the previous step for the resolution of the Poisson equation for `tggg` . More...

Scalar	ssjm1_khi
	Effective source at the previous step for the resolution of the Poisson equation for the scalar $\chi$ by means of `Map_et::poisson` . More...

Vector	ssjm1_wshift
	Effective source at the previous step for the resolution of the vector Poisson equation for . More...

double *	p_angu_mom
	Angular momentum. More...

double *	p_tsw
	Ratio T/W. More...

double *	p_grv2
	Error on the virial identity GRV2. More...

double *	p_grv3
	Error on the virial identity GRV3. More...

double *	p_r_circ
	Circumferential radius (equator) More...

double *	p_r_circ_merid
	Circumferential radius (meridian) More...

double *	p_aplat
	Flatening r_pole/r_eq. More...

double *	p_area
	Integrated surface area. More...

double *	p_z_eqf
	Forward redshift factor at equator. More...

double *	p_z_eqb
	Backward redshift factor at equator. More...

double *	p_z_pole
	Redshift factor at North pole. More...

double *	p_mom_quad
	Quadrupole moment. More...

double *	p_r_isco
	Circumferential radius of the ISCO. More...

double *	p_f_isco
	Orbital frequency of the ISCO. More...

double *	p_espec_isco
	Specific energy of a particle on the ISCO. More...

double *	p_lspec_isco
	Specific angular momentum of a particle on the ISCO. More...

double *	p_f_eq
	Orbital frequency at the equator. More...

Tbl *	p_surf_grav
	Surface gravity (along the theta direction) More...

Map &	mp
	Mapping associated with the star. More...

int	nzet
	Number of domains of `*mp` occupied by the star. More...

const Eos &	eos
	Equation of state of the stellar matter. More...

Scalar	ent
	Log-enthalpy. More...

Scalar	nbar
	Baryon density in the fluid frame. More...

Scalar	ener
	Total energy density in the fluid frame. More...

Scalar	press
	Fluid pressure. More...

Scalar	ener_euler
	Total energy density in the Eulerian frame. More...

Scalar	s_euler
	Trace of the stress scalar in the Eulerian frame. More...

Scalar	gam_euler
	Lorentz factor between the fluid and Eulerian observers. More...

Vector	u_euler
	Fluid 3-velocity with respect to the Eulerian observer. More...

Sym_tensor	stress_euler
	Spatial part of the stress-energy tensor with respect to the Eulerian observer. More...

Scalar	logn
	Logarithm of the lapse N . More...

Scalar	nn
	Lapse function N . More...

Vector	beta
	Shift vector. More...

Scalar	lnq

Metric	gamma
	3-metric More...

double *	p_ray_eq
	Coordinate radius at $\phi=0$ , $\theta=\pi/2$ . More...

double *	p_ray_eq_pis2
	Coordinate radius at $\phi=\pi/2$ , $\theta=\pi/2$ . More...

double *	p_ray_eq_pi
	Coordinate radius at $\phi=\pi$ , $\theta=\pi/2$ . More...

double *	p_ray_eq_3pis2
	Coordinate radius at $\phi=3\pi/2$ , $\theta=\pi/2$ . More...

double *	p_ray_pole
	Coordinate radius at $\theta=0$ . More...

Itbl *	p_l_surf
	Description of the stellar surface: 2-D `Itbl` containing the values of the domain index l on the surface at the collocation points in $(\theta', \phi')$ . More...

Tbl *	p_xi_surf
	Description of the stellar surface: 2-D `Tbl` containing the values of the radial coordinate $\xi$ on the surface at the collocation points in $(\theta', \phi')$ . More...

double *	p_mass_b
	Baryon mass. More...

double *	p_mass_g
	Gravitational mass. More...

Friends
ostream &	operator<< (ostream &, const Star &)
	Display. More...

Detailed Description

Class for differentially rotating stars in quasi-isotropic gauge and maximal slicing.

()

Definition at line 39 of file star_rot_diff.h.

Constructor & Destructor Documentation

◆ Star_rot_diff() [1/3]

Lorene::Star_rot_diff::Star_rot_diff	(	Map &	mp_i,
		int	nzet_i,
		bool	relat,
		const Eos &	eos_i,
		double(*)(double, const Tbl &)	omega_frot_i,
		double(*)(double, const Tbl &)	primfrot_i,
		const Tbl &	par_frot_i
	)

Standard constructor.

Parameters

mp_i	Mapping on which the star will be defined
nzet_i	Number of domains occupied by the star
relat	should be `true` for a relativistic star, `false` for a Newtonian one
eos_i	Equation of state of the stellar matter
omega_frot_i	Function $\Omega(F)$ defining the rotation profile.
primfrot_i	Primitive of $F\frac{d\Omega(F)}{dF}$ which vanishes at the stellar center
par_frot_i	Parameters of functions `omega_frot_i` and `primfrot_i` , `par_frot_i(0)` being the central value of $\Omega$ .

Definition at line 44 of file star_rot_diff.C.

References Lorene::Star_rot::omega, omega_field, omega_max, omega_min, and prim_field.

◆ Star_rot_diff() [2/3]

Lorene::Star_rot_diff::Star_rot_diff ( const Star_rot_diff & star )

Copy constructor.

Definition at line 69 of file star_rot_diff.C.

◆ Star_rot_diff() [3/3]

Lorene::Star_rot_diff::Star_rot_diff	(	Map &	mp_i,
		const Eos &	eos_i,
		FILE *	fich,
		double(*)(double, const Tbl &)	omega_frot_i,
		double(*)(double, const Tbl &)	primfrot_i
	)

Constructor from a file (see sauve(FILE*) ).

Parameters

mp_i	Mapping on which the star will be defined
eos_i	Equation of state of the stellar matter
fich	input file (must have been created by the function `sauve` )
omega_frot_i	Function $\Omega(F)$ defining the rotation profile.
primfrot_i	Primitive of $F\frac{d\Omega(F)}{dF}$ which vanishes at the stellar center

Definition at line 83 of file star_rot_diff.C.

References fait_prim_field(), Lorene::fread_be(), Lorene::Map::get_mg(), Lorene::Star::mp, omega_field, omega_max, and omega_min.

◆ ~Star_rot_diff()

Lorene::Star_rot_diff::~Star_rot_diff ( )

virtual

Destructor.

Definition at line 109 of file star_rot_diff.C.

Member Function Documentation

◆ angu_mom()

double Lorene::Star_rot::angu_mom ( ) const

virtualinherited

Angular momentum.

Definition at line 168 of file star_rot_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::b_car, Lorene::Star::ener_euler, Lorene::Scalar::get_spectral_va(), Lorene::Scalar::integrale(), Lorene::Scalar::mult_r(), Lorene::Star::nbar, Lorene::Star_rot::p_angu_mom, Lorene::Star::press, Lorene::Star_rot::relativistic, Lorene::Scalar::set_spectral_va(), and Lorene::Star_rot::uuu.

◆ aplat()

double Lorene::Star_rot::aplat ( ) const

virtualinherited

Flatening r_pole/r_eq.

Definition at line 489 of file star_rot_global.C.

References Lorene::Star_rot::p_aplat, Lorene::Star::ray_eq(), and Lorene::Star::ray_pole().

◆ area()

double Lorene::Star_rot::area ( ) const

virtualinherited

Integrated surface area in ${\rm km}^2$ .

Definition at line 429 of file star_rot_global.C.

References Lorene::Valeur::annule_hard(), Lorene::Valeur::c_cf, Lorene::Valeur::dsdt(), Lorene::Star_rot::get_a_car(), Lorene::Mg3d::get_angu(), Lorene::Star_rot::get_bbb(), Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Scalar::get_spectral_va(), Lorene::Star_rot::l_surf(), Lorene::Star::mp, Lorene::Valeur::mult_st(), Lorene::Star_rot::p_area, Lorene::sqrt(), Lorene::Valeur::std_base_scal(), Lorene::Valeur::val_point_jk(), Lorene::Map_radial::val_r_jk(), and Lorene::Star::xi_surf().

◆ del_deriv()

void Lorene::Star_rot::del_deriv ( ) const

protectedvirtualinherited

Deletes all the derived quantities.

Reimplemented from Lorene::Star.

Definition at line 310 of file star_rot.C.

◆ del_hydro_euler()

void Lorene::Star_rot::del_hydro_euler ( )

protectedvirtualinherited

Sets to ETATNONDEF (undefined state) the hydrodynamical quantities relative to the Eulerian observer.

Reimplemented from Lorene::Star.

Definition at line 362 of file star_rot.C.

References Lorene::Star_rot::del_deriv(), and Lorene::Star::del_hydro_euler().

◆ display_poly()

void Lorene::Star_rot_diff::display_poly ( ostream & ost ) const

virtual

Display in polytropic units.

Reimplemented from Lorene::Star_rot.

Definition at line 232 of file star_rot_diff.C.

References Lorene::Star_rot::display_poly(), Lorene::Star::ener, Lorene::Star::eos, Lorene::Eos_poly::get_gam(), Lorene::Eos_poly::get_kap(), Lorene::Map::get_mg(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), Lorene::max(), Lorene::Star::mp, Lorene::Star::nbar, Lorene::Star::nzet, omega_field, omega_max, omega_min, Lorene::pow(), Lorene::sqrt(), and Lorene::Scalar::val_grid_point().

◆ equation_of_state()

void Lorene::Star::equation_of_state ( )

inherited

Computes the proper baryon and energy density, as well as pressure from the enthalpy.

Definition at line 465 of file star.C.

References Lorene::Param::add_int(), Lorene::Scalar::allocate_all(), Lorene::Star::del_deriv(), Lorene::Star::ener, Lorene::Eos::ener_ent(), Lorene::Star::ent, Lorene::Star::eos, Lorene::Mg3d::get_grille3d(), Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_nzone(), Lorene::Star::mp, Lorene::Star::nbar, Lorene::Eos::nbar_ent(), Lorene::Star::nzet, Lorene::Star::press, Lorene::Eos::press_ent(), Lorene::Mtbl::set(), Lorene::Scalar::set_domain(), Lorene::Mtbl::set_etat_qcq(), Lorene::Tbl::set_etat_qcq(), Lorene::Scalar::set_etat_qcq(), Lorene::Scalar::std_spectral_base(), Lorene::Mtbl::t, and Lorene::Grille3d::x.

◆ equilibrium()

void Lorene::Star_rot_diff::equilibrium	(	double	ent_c,
		double	omega0,
		double	fact_omega,
		int	nzadapt,
		const Tbl &	ent_limit,
		const Itbl &	icontrol,
		const Tbl &	control,
		double	mbar_wanted,
		double	aexp_mass,
		Tbl &	diff,
		Param *	= `0x0`
	)

virtual

Computes an equilibrium configuration.

Parameters

ent_c	[input] Central enthalpy
omega0	[input] Requested central angular velocity (if `fact_omega=1`. )
fact_omega	[input] 1.01 = search for the Keplerian frequency, = otherwise.
nzadapt	[input] Number of (inner) domains where the mapping adaptation to an iso-enthalpy surface should be performed
ent_limit	[input] 1-D `Tbl` of dimension `nzet` which defines the enthalpy at the outer boundary of each domain
icontrol	[input] Set of integer parameters (stored as a 1-D `Itbl` of size 9) to control the iteration: `icontrol(0)` = mer_max : maximum number of steps `icontrol(1)` = mer_rot : step at which the rotation is switched on `icontrol(2)` = mer_change_omega : step at which the rotation velocity is changed to reach the final one `icontrol(3)` = mer_fix_omega : step at which the final rotation velocity must have been reached `icontrol(4)` = mer_mass : the absolute value of `mer_mass` is the step from which the baryon mass is forced to converge, by varying the central enthalpy (`mer_mass` > 0 ) or the angular velocity (`mer_mass` < 0 ) `icontrol(5)` = mermax_poisson : maximum number of steps in `Map_et::poisson` `icontrol(6)` = mer_triax : step at which the 3-D perturbation is switched on `icontrol(7)` = delta_mer_kep : number of steps after `mer_fix_omega` when `omega` starts to be increased by `fact_omega` to search for the Keplerian velocity `icontrol(8)` = mer_diff : step at which differential rotation is switched on
control	[input] Set of parameters (stored as a 1-D `Tbl` of size 7) to control the iteration: `control(0)` = precis : threshold on the enthalpy relative change for ending the computation `control(1)` = omega_ini : initial central angular velocity, switched on only if `mer_rot` < 0 , otherwise 0 is used `control(2)` = relax : relaxation factor in the main iteration `control(3)` = relax_poisson : relaxation factor in `Map_et::poisson` `control(4)` = thres_adapt : threshold on dH/dr for freezing the adaptation of the mapping `control(5)` = ampli_triax : relative amplitude of the 3-D perturbation `control(6)` = precis_adapt : precision for `Map_et::adapt`
mbar_wanted	[input] Requested baryon mass (effective only if `mer_mass` > mer_max )
aexp_mass	[input] Exponent for the increase factor of the central enthalpy to converge to the requested baryon mass
diff	[output] 1-D `Tbl` of size 7 for the storage of some error indicators : `diff(0)` : Relative change in the enthalpy field between two successive steps `diff(1)` : Relative error in the resolution of the Poisson equation for `nuf` `diff(2)` : Relative error in the resolution of the Poisson equation for `nuq` `diff(3)` : Relative error in the resolution of the Poisson equation for `dzeta` `diff(4)` : Relative error in the resolution of the Poisson equation for `tggg` `diff(5)` : Relative error in the resolution of the equation for `shift` (x comp.) `diff(6)` : Relative error in the resolution of the equation for `shift` (y comp.)

Reimplemented from Lorene::Star_rot.

Definition at line 42 of file strot_diff_equil.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_nzone(), Lorene::Mg3d::get_type_t(), and Lorene::Star::mp.

◆ equilibrium_spher()

void Lorene::Star::equilibrium_spher	(	double	ent_c,
		double	precis = `1.e-14`,
		const Tbl *	pent_limit = `0x0`
	)

virtualinherited

Computes a spherical static configuration.

Parameters

ent_c	[input] central value of the enthalpy
precis	[input] threshold in the relative difference between the enthalpy fields of two consecutive steps to stop the iterative procedure (default value: 1.e-14)
ent_limit	[input] : array of enthalpy values to be set at the boundaries between the domains; if set to 0x0 (default), the initial values will be kept.

Definition at line 101 of file star_equil_spher.C.

References Lorene::Star_rot::a_car, Lorene::Map_et::adapt(), Lorene::Param::add_double(), Lorene::Param::add_int(), Lorene::Param::add_int_mod(), Lorene::Param::add_tbl(), Lorene::Scalar::annule(), Lorene::Star_rot::b_car, Lorene::Star_rot::bbb, Lorene::diffrel(), Lorene::Scalar::dsdr(), Lorene::Map_af::dsdr(), Lorene::Star_rot::dzeta, Lorene::Star::ener, Lorene::Star::ener_euler, Lorene::Star::ent, Lorene::Star::equation_of_state(), Lorene::exp(), Lorene::Star::gam_euler, Lorene::Star::gamma, Lorene::Map_af::get_alpha(), Lorene::Map_et::get_alpha(), Lorene::Map_af::get_beta(), Lorene::Map_et::get_beta(), Lorene::Map::get_bvect_cart(), Lorene::Map::get_mg(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_nzone(), Lorene::Map_af::homothetie(), Lorene::Scalar::integrale(), Lorene::Star::logn, Lorene::Star::mass_b(), Lorene::Star::mass_g(), Lorene::Star::mp, Lorene::Star::nn, Lorene::norme(), Lorene::Star::nzet, Lorene::Map_af::poisson(), Lorene::Star::press, Lorene::Star::s_euler, Lorene::Vector::set(), Lorene::Map_af::set_alpha(), Lorene::Map_af::set_beta(), Lorene::Scalar::set_dzpuis(), Lorene::Cmp::set_etat_qcq(), Lorene::Tensor::set_etat_zero(), Lorene::sqrt(), Lorene::Scalar::std_spectral_base(), Lorene::Star::u_euler, Lorene::Scalar::val_grid_point(), and Lorene::Map::val_r().

◆ espec_isco()

double Lorene::Star_rot::espec_isco ( ) const

virtualinherited

Energy of a particle on the ISCO.

Definition at line 292 of file star_rot_isco.C.

References Lorene::Star_rot::p_espec_isco, and Lorene::Star_rot::r_isco().

◆ extrinsic_curvature()

void Lorene::Star_rot::extrinsic_curvature ( )

inherited

Computes tkij and ak_car from shift , nnn and b_car .

Definition at line 113 of file star_rot_upmetr.C.

References Lorene::Scalar::dsdr(), Lorene::Scalar::get_etat(), Lorene::Map::get_mg(), Lorene::Star::mp, Lorene::Star_rot::nphi, Lorene::Tensor::set_etat_zero(), Lorene::Scalar::srdsdt(), and Lorene::Star_rot::tkij.

◆ f_eq()

double Lorene::Star_rot::f_eq ( ) const

virtualinherited

Orbital frequency at the equator.

Definition at line 310 of file star_rot_isco.C.

References Lorene::Star_rot::p_f_eq, and Lorene::Star_rot::r_isco().

◆ f_isco()

double Lorene::Star_rot::f_isco ( ) const

virtualinherited

Orbital frequency at the innermost stable circular orbit (ISCO).

Definition at line 258 of file star_rot_isco.C.

References Lorene::Star_rot::p_f_isco, and Lorene::Star_rot::r_isco().

◆ fait_nphi()

void Lorene::Star_rot::fait_nphi ( )

inherited

Computes tnphi and nphi from the Cartesian components of the shift, stored in shift .

Definition at line 779 of file star_rot.C.

References Lorene::Star::beta.

◆ fait_omega_field()

void Lorene::Star_rot_diff::fait_omega_field	(	double	omeg_min,
		double	omeg_max,
		double	precis,
		int	nitermax
	)

Computes $\Omega(r,\theta)$ (member omega_field ).

The computation amounts to solving the equation

$\Omega - \Omega\left({B^2 r^2\sin^2\theta (\Omega - N^\varphi) \over N^2 - B^2 r^2 \sin^2(\Omega-N^\varphi)^2}\right) = 0$

for $\Omega$ .

Parameters

omeg_min	[input] Lower bound of the interval for searching omega
omeg_max	[input] Higher bound of the interval for searching omega
precis	[input] Required precision in the determination of the zero by the secant method
nitermax	[input] Maximum number of iterations in the secant method to compute the zero.

Definition at line 43 of file strot_diff_faitomeg.C.

References Lorene::Param::add_int(), Lorene::Param::add_scalar(), Lorene::Param::add_star(), Lorene::Tensor::annule_domain(), Lorene::Star_rot::bbb, Lorene::Scalar::get_etat(), Lorene::Map::get_mg(), Lorene::Mg3d::get_nzone(), Lorene::Star::mp, Lorene::Scalar::mult_rsint(), Lorene::Star::nn, Lorene::Star_rot::nphi, omega_field, and Lorene::Scalar::std_spectral_base().

◆ fait_prim_field()

void Lorene::Star_rot_diff::fait_prim_field ( )

Computes the member prim_field from omega_field .

Definition at line 177 of file strot_diff_faitomeg.C.

References Lorene::Scalar::allocate_all(), Lorene::Tensor::annule_domain(), Lorene::Star_rot::bbb, Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_nzone(), Lorene::Star::mp, Lorene::Scalar::mult_rsint(), Lorene::Star::nn, Lorene::Star_rot::nphi, Lorene::Star::nzet, omega_field, par_frot, prim_field, primfrot, Lorene::Tbl::set(), Lorene::Scalar::set_domain(), Lorene::Scalar::std_spectral_base(), and Lorene::Scalar::val_grid_point().

◆ fait_shift()

void Lorene::Star_rot::fait_shift ( )

inherited

Computes shift from w_shift and khi_shift according to Shibata's prescription [Prog.

Theor. Phys. 101 , 1199 (1999)] :

$N^i = {7\over 8} W^i - {1\over 8} \left(\nabla^i\chi+\nabla^iW^kx_k\right)$

Definition at line 730 of file star_rot.C.

References Lorene::Star::beta, Lorene::contract(), Lorene::Map::cosp, Lorene::Map::cost, Lorene::Tensor::dec_dzpuis(), Lorene::Tensor::derive_con(), Lorene::Scalar::derive_con(), Lorene::Scalar::domain(), Lorene::Map::flat_met_cart(), Lorene::Map::get_bvect_cart(), Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nzone(), Lorene::Star_rot::khi_shift, Lorene::Star::mp, Lorene::Tbl::set(), Lorene::Vector::set(), Lorene::Tensor::set(), Lorene::Scalar::set_domain(), Lorene::Map::sinp, Lorene::Map::sint, Lorene::Star_rot::w_shift, Lorene::Map::x, Lorene::Map::y, and Lorene::Map::z.

◆ get_a_car()

const Scalar& Lorene::Star_rot::get_a_car ( ) const

inlineinherited

Returns the square of the metric factor A.

Definition at line 333 of file star_rot.h.

References Lorene::Star_rot::a_car.

◆ get_ak_car()

const Scalar& Lorene::Star_rot::get_ak_car ( ) const

inlineinherited

Returns the scalar $A^2 K_{ij} K^{ij}$ .

For axisymmetric stars, this quantity is related to the derivatives of $N^\varphi$ by

$A^2 K_{ij} K^{ij} = {B^2 \over 2 N^2} \, r^2\sin^2\theta \, \left[ \left( {\partial N^\varphi \over \partial r} \right) ^2 + {1\over r^2} \left( {\partial N^\varphi \over \partial \theta} \right) ^2 \right] \ .$

In particular it is related to the quantities $k_1$ and $k_2$ introduced by Eqs. (3.7) and (3.8) of Bonazzola et al. Astron. Astrophys. 278 , 421 (1993) by

$A^2 K_{ij} K^{ij} = 2 A^2 (k_1^2 + k_2^2) \ .$

Definition at line 417 of file star_rot.h.

References Lorene::Star_rot::ak_car.

◆ get_b_car()

const Scalar& Lorene::Star_rot::get_b_car ( ) const

inlineinherited

Returns the square of the metric factor B.

Definition at line 336 of file star_rot.h.

References Lorene::Star_rot::b_car.

◆ get_bbb()

const Scalar& Lorene::Star_rot::get_bbb ( ) const

inlineinherited

Returns the metric factor B.

Definition at line 330 of file star_rot.h.

References Lorene::Star_rot::bbb.

◆ get_beta()

const Vector& Lorene::Star::get_beta ( ) const

inlineinherited

Returns the shift vector $\beta^i$ .

Definition at line 402 of file star.h.

References Lorene::Star::beta.

◆ get_dzeta()

const Scalar& Lorene::Star_rot::get_dzeta ( ) const

inlineinherited

Returns the Metric potential $\zeta = \ln(AN)$ .

Definition at line 360 of file star_rot.h.

References Lorene::Star_rot::dzeta.

◆ get_ener()

const Scalar& Lorene::Star::get_ener ( ) const

inlineinherited

Returns the proper total energy density.

Definition at line 370 of file star.h.

References Lorene::Star::ener.

◆ get_ener_euler()

const Scalar& Lorene::Star::get_ener_euler ( ) const

inlineinherited

Returns the total energy density with respect to the Eulerian observer.

Definition at line 376 of file star.h.

References Lorene::Star::ener_euler.

◆ get_ent()

const Scalar& Lorene::Star::get_ent ( ) const

inlineinherited

Returns the enthalpy field.

Definition at line 364 of file star.h.

References Lorene::Star::ent.

◆ get_eos()

const Eos& Lorene::Star::get_eos ( ) const

inlineinherited

Returns the equation of state.

Definition at line 361 of file star.h.

References Lorene::Star::eos.

◆ get_gam_euler()

const Scalar& Lorene::Star::get_gam_euler ( ) const

inlineinherited

Returns the Lorentz factor between the fluid and Eulerian observers.

Definition at line 382 of file star.h.

References Lorene::Star::gam_euler.

◆ get_gamma()

const Metric& Lorene::Star::get_gamma ( ) const

inlineinherited

Returns the 3-metric $\gamma$ .

Definition at line 409 of file star.h.

References Lorene::Star::gamma.

◆ get_khi_shift()

const Scalar& Lorene::Star_rot::get_khi_shift ( ) const

inlineinherited

Returns the scalar $\chi$ used in the decomposition of shift
following Shibata's prescription [Prog.

Theor. Phys. 101 , 1199 (1999)] :

$N^i = {7\over 8} W^i - {1\over 8} \left(\nabla^i\chi+\nabla^iW^kx_k\right)$

NB: w_shift contains the components of $W^i$ with respect to the Cartesian triad associated with the mapping mp .

Definition at line 391 of file star_rot.h.

References Lorene::Star_rot::khi_shift.

◆ get_logn()

const Scalar& Lorene::Star::get_logn ( ) const

inlineinherited

Returns the logarithm of the lapse N.

In the Newtonian case, this is the Newtonian gravitational potential (in units of $c^2$ ).

Definition at line 396 of file star.h.

References Lorene::Star::logn.

◆ get_mp()

const Map& Lorene::Star::get_mp ( ) const

inlineinherited

Returns the mapping.

Definition at line 355 of file star.h.

References Lorene::Star::mp.

◆ get_nbar()

const Scalar& Lorene::Star::get_nbar ( ) const

inlineinherited

Returns the proper baryon density.

Definition at line 367 of file star.h.

References Lorene::Star::nbar.

◆ get_nn()

const Scalar& Lorene::Star::get_nn ( ) const

inlineinherited

Returns the lapse function N.

Definition at line 399 of file star.h.

References Lorene::Star::nn.

◆ get_nphi()

const Scalar& Lorene::Star_rot::get_nphi ( ) const

inlineinherited

Returns the metric coefficient $N^\varphi$ .

Definition at line 339 of file star_rot.h.

References Lorene::Star_rot::nphi.

◆ get_nuf()

const Scalar& Lorene::Star_rot::get_nuf ( ) const

inlineinherited

Returns the part of the Metric potential $\nu = \ln N$ = logn generated by the matter terms.

Definition at line 352 of file star_rot.h.

References Lorene::Star_rot::nuf.

◆ get_nuq()

const Scalar& Lorene::Star_rot::get_nuq ( ) const

inlineinherited

Returns the Part of the Metric potential $\nu = \ln N$ = logn generated by the quadratic terms.

Definition at line 357 of file star_rot.h.

References Lorene::Star_rot::nuq.

◆ get_nzet()

int Lorene::Star::get_nzet ( ) const

inlineinherited

Returns the number of domains occupied by the star.

Definition at line 358 of file star.h.

References Lorene::Star::nzet.

◆ get_omega_c()

double Lorene::Star_rot_diff::get_omega_c ( ) const

virtual

Returns the central value of the rotation angular velocity ([f_unit] )

Reimplemented from Lorene::Star_rot.

Definition at line 289 of file star_rot_diff.C.

References omega_field, and Lorene::Scalar::val_grid_point().

◆ get_omega_field()

const Scalar& Lorene::Star_rot_diff::get_omega_field ( ) const

inline

Returns the angular velocity field $\Omega$ .

Definition at line 138 of file star_rot_diff.h.

References omega_field.

◆ get_press()

const Scalar& Lorene::Star::get_press ( ) const

inlineinherited

Returns the fluid pressure.

Definition at line 373 of file star.h.

References Lorene::Star::press.

◆ get_s_euler()

const Scalar& Lorene::Star::get_s_euler ( ) const

inlineinherited

Returns the trace of the stress tensor in the Eulerian frame.

Definition at line 379 of file star.h.

References Lorene::Star::s_euler.

◆ get_stress_euler()

const Tensor& Lorene::Star::get_stress_euler ( ) const

inlineinherited

Returns the spatial part of the stress-energy tensor with respect to the Eulerian observer.

Definition at line 390 of file star.h.

References Lorene::Star::stress_euler.

◆ get_tggg()

const Scalar& Lorene::Star_rot::get_tggg ( ) const

inlineinherited

Returns the Metric potential $\tilde G = (NB-1) r\sin\theta$ .

Definition at line 363 of file star_rot.h.

References Lorene::Star_rot::tggg.

◆ get_tkij()

const Sym_tensor& Lorene::Star_rot::get_tkij ( ) const

inlineinherited

Returns the tensor ${\tilde K_{ij}}$ related to the extrinsic curvature tensor by ${\tilde K_{ij}} = B^{-2} K_{ij}$ .

tkij contains the Cartesian components of ${\tilde K_{ij}}$ .

Definition at line 398 of file star_rot.h.

References Lorene::Star_rot::tkij.

◆ get_tnphi()

const Scalar& Lorene::Star_rot::get_tnphi ( ) const

inlineinherited

Returns the component $\tilde N^\varphi = N^\varphi r\sin\theta$ of the shift vector.

Definition at line 344 of file star_rot.h.

References Lorene::Star_rot::tnphi.

◆ get_u_euler()

const Vector& Lorene::Star::get_u_euler ( ) const

inlineinherited

Returns the fluid 3-velocity with respect to the Eulerian observer.

Definition at line 385 of file star.h.

References Lorene::Star::u_euler.

◆ get_uuu()

const Scalar& Lorene::Star_rot::get_uuu ( ) const

inlineinherited

Returns the norm of u_euler.

Definition at line 347 of file star_rot.h.

References Lorene::Star_rot::uuu.

◆ get_w_shift()

const Vector& Lorene::Star_rot::get_w_shift ( ) const

inlineinherited

Returns the vector $W^i$ used in the decomposition of shift , following Shibata's prescription [Prog.

Theor. Phys. 101 , 1199 (1999)] :

$N^i = {7\over 8} W^i - {1\over 8} \left(\nabla^i\chi+\nabla^iW^kx_k\right)$

NB: w_shift contains the components of $W^i$ with respect to the Cartesian triad associated with the mapping mp .

Definition at line 377 of file star_rot.h.

References Lorene::Star_rot::w_shift.

◆ grv2()

double Lorene::Star_rot::grv2 ( ) const

virtualinherited

Error on the virial identity GRV2.

This indicator is only valid for relativistic computations.

Definition at line 222 of file star_rot_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::ak_car, Lorene::Scalar::derive_cov(), Lorene::Star::ener_euler, Lorene::Map::flat_met_spher(), Lorene::Star_rot::lambda_grv2(), Lorene::Star::logn, Lorene::Star::mp, Lorene::Star::nbar, Lorene::Star_rot::p_grv2, Lorene::Star::press, Lorene::Star_rot::relativistic, and Lorene::Star_rot::uuu.

◆ grv3()

double Lorene::Star_rot::grv3 ( ostream * ost = 0x0 ) const

virtualinherited

Error on the virial identity GRV3.

The error is computed as the integral defined by Eq. (43) of [Gourgoulhon and Bonazzola, Class. Quantum Grav. 11, 443 (1994)] divided by the integral of the matter terms.

Parameters

ost	output stream to give details of the computation; if set to 0x0 [default value], no details will be given.

Definition at line 253 of file star_rot_global.C.

References Lorene::Star_rot::ak_car, Lorene::Star_rot::bbb, Lorene::Scalar::derive_cov(), Lorene::Star_rot::dzeta, Lorene::Map::flat_met_spher(), Lorene::Scalar::get_etat(), Lorene::log(), Lorene::Star::logn, Lorene::Star::mp, Lorene::Star_rot::p_grv3, Lorene::Star_rot::relativistic, Lorene::Scalar::srdsdt(), and Lorene::Scalar::std_spectral_base().

◆ hydro_euler()

void Lorene::Star_rot_diff::hydro_euler ( )

virtual

Computes the hydrodynamical quantities relative to the Eulerian observer from those in the fluid frame.

The calculation is performed starting from the quantities omega_field , ent , ener , press , and a_car ,
which are supposed to be up to date.
From these, the following fields are updated: gam_euler , u_euler , ener_euler , s_euler .

Reimplemented from Lorene::Star_rot.

Definition at line 38 of file strot_diff_hydro.C.

References Lorene::Tensor::annule_domain(), Lorene::Star::beta, Lorene::Map::get_bvect_cart(), Lorene::Map::get_bvect_spher(), Lorene::Valeur::get_etat(), Lorene::Map::get_mg(), Lorene::Mg3d::get_nzone(), Lorene::Star::mp, Lorene::Star::nn, Lorene::Star_rot::nphi, omega_field, Lorene::Valeur::set(), Lorene::Vector::set(), Lorene::Tensor::set(), Lorene::Tensor::set_etat_qcq(), Lorene::Tensor::set_triad(), Lorene::Vector::std_spectral_base(), Lorene::Star::u_euler, Lorene::Map::x, and Lorene::Map::y.

◆ is_relativistic()

bool Lorene::Star_rot::is_relativistic ( ) const

inlineinherited

Returns true for a relativistic star, false for a Newtonian one.

Definition at line 322 of file star_rot.h.

References Lorene::Star_rot::relativistic.

◆ l_surf()

const Itbl & Lorene::Star_rot::l_surf ( ) const

virtualinherited

Description of the stellar surface: returns a 2-D Itbl containing the values of the domain index l on the surface at the collocation points in $(\theta', \phi')$ .

The stellar surface is defined as the location where the enthalpy (member ent ) vanishes.

Reimplemented from Lorene::Star.

Definition at line 86 of file star_rot_global.C.

References Lorene::Star::ent, Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Scalar::get_spectral_va(), Lorene::Star::mp, Lorene::Star::nzet, Lorene::Star::p_l_surf, and Lorene::Star::p_xi_surf.

◆ lambda_grv2()

double Lorene::Star_rot::lambda_grv2	(	const Scalar &	sou_m,
		const Scalar &	sou_q
	)

staticinherited

Computes the coefficient $\lambda$ which ensures that the GRV2 virial identity is satisfied.

$\lambda$ is the coefficient by which one must multiply the quadratic source term $\sigma_q$ of the 2-D Poisson equation

$\Delta_2 u = \sigma_m + \sigma_q$

in order that the total source does not contain any monopolar term, i.e. in order that

$\int_0^{2\pi} \int_0^{+\infty} \sigma(r, \theta) \, r \, dr \, d\theta = 0 \ ,$

where $\sigma = \sigma_m + \sigma_q$ . $\lambda$ is computed according to the formula

$\lambda = - { \int_0^{2\pi} \int_0^{+\infty} \sigma_m(r, \theta) \, r \, dr \, d\theta \over \int_0^{2\pi} \int_0^{+\infty} \sigma_q(r, \theta) \, r \, dr \, d\theta } \ .$

Then, by construction, the new source $\sigma' = \sigma_m + \lambda \sigma_q$ has a vanishing monopolar term.

Parameters

sou_m	[input] matter source term $\sigma_m$
sou_q	[input] quadratic source term $\sigma_q$

Returns: value of $\lambda$

Definition at line 69 of file star_rot_lambda_grv2.C.

References Lorene::Scalar::check_dzpuis(), Lorene::Map::get_mg(), Lorene::Tensor::get_mp(), Lorene::Mg3d::get_nzone(), Lorene::Mg3d::get_type_r(), and Lorene::Map::val_r().

◆ lspec_isco()

double Lorene::Star_rot::lspec_isco ( ) const

virtualinherited

Angular momentum of a particle on the ISCO.

Definition at line 275 of file star_rot_isco.C.

References Lorene::Star_rot::p_lspec_isco, and Lorene::Star_rot::r_isco().

◆ mass_b()

double Lorene::Star_rot::mass_b ( ) const

virtualinherited

Baryon mass.

Implements Lorene::Star.

Definition at line 116 of file star_rot_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::bbb, Lorene::Star::gam_euler, Lorene::Scalar::get_etat(), Lorene::Scalar::integrale(), Lorene::Star::nbar, Lorene::Star::p_mass_b, and Lorene::Star_rot::relativistic.

◆ mass_g()

double Lorene::Star_rot::mass_g ( ) const

virtualinherited

Gravitational mass.

Implements Lorene::Star.

Definition at line 142 of file star_rot_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::bbb, Lorene::Star::ener_euler, Lorene::Star_rot::mass_b(), Lorene::Star::nn, Lorene::Star::p_mass_g, Lorene::Star::press, Lorene::Star_rot::relativistic, Lorene::Star::s_euler, Lorene::Scalar::std_spectral_base(), Lorene::Star_rot::tnphi, and Lorene::Star_rot::uuu.

◆ mean_radius()

double Lorene::Star_rot::mean_radius ( ) const

virtualinherited

Mean star radius from the area $r_{\rm mean} = \sqrt{\mathcal{A}} / 4\pi$ .

Definition at line 479 of file star_rot_global.C.

References Lorene::Star_rot::area(), and Lorene::sqrt().

◆ mom_quad()

double Lorene::Star_rot::mom_quad ( ) const

virtualinherited

Quadrupole moment.

The quadrupole moment Q is defined according to Eq. (7) of [Salgado, Bonazzola, Gourgoulhon and Haensel, Astron. Astrophys. 291 , 155 (1994)]. At the Newtonian limit it is related to the component ${\bar I}_{zz}$ of the MTW (1973) reduced quadrupole moment ${\bar I}_{ij}$ by: $Q = -3/2 {\bar I}_{zz}$ . Note that Q is the negative of the quadrupole moment defined by Laarakkers and Poisson, Astrophys. J. 512 , 282 (1999).

Definition at line 586 of file star_rot_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::ak_car, Lorene::Star_rot::bbb, Lorene::Scalar::check_dzpuis(), Lorene::Scalar::derive_cov(), Lorene::Star::ener_euler, Lorene::Map::flat_met_spher(), Lorene::Scalar::get_etat(), Lorene::Scalar::inc_dzpuis(), Lorene::log(), Lorene::Star::logn, Lorene::Star::mp, Lorene::Scalar::mult_r(), Lorene::Star::nbar, Lorene::Star_rot::p_mom_quad, Lorene::Star_rot::relativistic, Lorene::Star::s_euler, and Lorene::Scalar::std_spectral_base().

◆ omega_funct()

double Lorene::Star_rot_diff::omega_funct ( double F ) const

Evaluates $\Omega(F)$ , where F is linked to the components of the fluid 4-velocity by

$F = u^t u_\varphi \ .$

.

omega_funct calls frot with the parameters par_frot .

Parameters

F	[input] value of

Returns: value of $\Omega(F))$

Definition at line 277 of file star_rot_diff.C.

References omega_frot, and par_frot.

◆ operator=()

void Lorene::Star_rot_diff::operator= ( const Star_rot_diff & star )

Assignment to another Star_rot_diff.

Definition at line 119 of file star_rot_diff.C.

References omega_field, omega_frot, omega_max, omega_min, Lorene::Star_rot::operator=(), par_frot, prim_field, and primfrot.

◆ operator>>()

ostream & Lorene::Star_rot_diff::operator>> ( ostream & ost ) const

protectedvirtual

Operator >> (virtual function called by the operator <<).

Reimplemented from Lorene::Star_rot.

Definition at line 161 of file star_rot_diff.C.

References Lorene::Star_rot::angu_mom(), Lorene::Star_rot::aplat(), display_poly(), Lorene::Star::ener, Lorene::Map::get_mg(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), get_omega_c(), Lorene::Star_rot::mass_b(), Lorene::Star_rot::mass_g(), Lorene::max(), Lorene::Star::mp, Lorene::Star::nbar, Lorene::Star::nzet, omega_field, omega_max, omega_min, Lorene::Star_rot::operator>>(), par_frot, Lorene::pow(), Lorene::Star::press, Lorene::Star::ray_eq(), Lorene::sqrt(), tsw(), and Lorene::Scalar::val_grid_point().

◆ partial_display()

void Lorene::Star_rot::partial_display ( ostream & ost ) const

protectedvirtualinherited

Printing of some informations, excluding all global quantities.

Definition at line 613 of file star_rot.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::aplat(), Lorene::Star_rot::b_car, Lorene::Star_rot::dzeta, Lorene::Star::ener, Lorene::Star::ent, Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nr(), Lorene::Mg3d::get_nt(), Lorene::Star_rot::get_omega_c(), Lorene::Star::logn, Lorene::Star::mp, Lorene::Star::nbar, Lorene::Star::nn, Lorene::Star_rot::nphi, Lorene::Star::nzet, Lorene::Star::press, Lorene::Star_rot::r_circ(), Lorene::Star_rot::r_circ_merid(), Lorene::Star::ray_eq(), Lorene::Star_rot::uuu, and Lorene::Scalar::val_grid_point().

◆ prim_funct_omega()

double Lorene::Star_rot_diff::prim_funct_omega ( double F ) const

Evaluates the primitive of $F\frac{d\Omega(F)}{dF}$ .

Parameters

F	[input] value of

Returns: value of $\int_0^F F'\,\frac{d\Omega(F')}{dF'} \, dF'$

Definition at line 283 of file star_rot_diff.C.

References par_frot, and primfrot.

◆ r_circ()

double Lorene::Star_rot::r_circ ( ) const

virtualinherited

Circumferential equatorial radius.

Definition at line 360 of file star_rot_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star_rot::p_r_circ.

◆ r_circ_merid()

double Lorene::Star_rot::r_circ_merid ( ) const

virtualinherited

Crcumferential meridional radius.

Definition at line 380 of file star_rot_global.C.

References Lorene::Valeur::annule_hard(), Lorene::Valeur::dsdt(), Lorene::Star_rot::get_a_car(), Lorene::Mg3d::get_angu(), Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Scalar::get_spectral_va(), Lorene::Star_rot::l_surf(), Lorene::Star::mp, Lorene::Star_rot::p_r_circ_merid, Lorene::sqrt(), Lorene::Valeur::std_base_scal(), Lorene::Cmp::std_base_scal(), Lorene::Valeur::val_point_jk(), Lorene::Map_radial::val_r_jk(), and Lorene::Star::xi_surf().

◆ r_isco()

double Lorene::Star_rot::r_isco ( ostream * ost = 0x0 ) const

virtualinherited

Circumferential radius of the innermost stable circular orbit (ISCO).

Parameters

ost	output stream to give details of the computation; if set to 0x0 [default value], no details will be given.

Definition at line 74 of file star_rot_isco.C.

References Lorene::Param::add_int(), Lorene::Param::add_scalar(), Lorene::Tensor::annule_domain(), Lorene::Star_rot::bbb, Lorene::Scalar::dsdr(), Lorene::Map::get_mg(), Lorene::Mg3d::get_nzone(), Lorene::Scalar::get_spectral_va(), Lorene::Star::mp, Lorene::Star::nn, Lorene::Star_rot::nphi, Lorene::Star::nzet, Lorene::Star_rot::p_espec_isco, Lorene::Star_rot::p_f_eq, Lorene::Star_rot::p_f_isco, Lorene::Star_rot::p_lspec_isco, Lorene::Star_rot::p_r_isco, Lorene::Map::r, Lorene::Star::ray_eq(), Lorene::sqrt(), Lorene::Scalar::std_spectral_base(), Lorene::Valeur::val_point(), Lorene::Map::val_r(), and Lorene::zerosec().

◆ ray_eq()

double Lorene::Star::ray_eq ( ) const

inherited

Coordinate radius at $\phi=0$ , $\theta=\pi/2$ [r_unit].

Definition at line 111 of file star_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_type_p(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star::p_ray_eq.

◆ ray_eq_3pis2()

double Lorene::Star::ray_eq_3pis2 ( ) const

inherited

Coordinate radius at $\phi=3\pi/2$ , $\theta=\pi/2$ [r_unit].

Definition at line 236 of file star_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_type_p(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star::p_ray_eq_3pis2.

◆ ray_eq_pi()

double Lorene::Star::ray_eq_pi ( ) const

inherited

Coordinate radius at $\phi=\pi$ , $\theta=\pi/2$ [r_unit].

Definition at line 189 of file star_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_type_p(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star::p_ray_eq_pi.

◆ ray_eq_pis2()

double Lorene::Star::ray_eq_pis2 ( ) const

inherited

Coordinate radius at $\phi=\pi/2$ , $\theta=\pi/2$ [r_unit].

Definition at line 141 of file star_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_np(), Lorene::Mg3d::get_nt(), Lorene::Mg3d::get_type_p(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star::p_ray_eq_pis2.

◆ ray_pole()

double Lorene::Star::ray_pole ( ) const

inherited

Coordinate radius at $\theta=0$ [r_unit].

Definition at line 281 of file star_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star::p_ray_pole.

◆ sauve()

void Lorene::Star_rot_diff::sauve ( FILE * fich ) const

virtual

Save in a file.

Reimplemented from Lorene::Star_rot.

Definition at line 144 of file star_rot_diff.C.

References Lorene::fwrite_be(), omega_field, omega_max, omega_min, par_frot, Lorene::Star::sauve(), Lorene::Tbl::sauve(), and Lorene::Scalar::sauve().

◆ set_der_0x0()

void Lorene::Star_rot::set_der_0x0 ( ) const

protectedvirtualinherited

Sets to 0x0 all the pointers on derived quantities.

Reimplemented from Lorene::Star.

Definition at line 337 of file star_rot.C.

◆ set_enthalpy()

void Lorene::Star::set_enthalpy ( const Scalar & ent_i )

inherited

Assignment of the enthalpy field.

Definition at line 382 of file star.C.

References Lorene::Star::del_deriv(), Lorene::Star::ent, and Lorene::Star::equation_of_state().

◆ set_mp()

Map& Lorene::Star::set_mp ( )

inlineinherited

Read/write of the mapping.

Definition at line 322 of file star.h.

References Lorene::Star::mp.

◆ surf_grav()

const Tbl & Lorene::Star_rot::surf_grav ( ) const

virtualinherited

Surface gravity (table along the theta direction)

Definition at line 671 of file star_rot_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star_rot::p_surf_grav.

◆ tsw()

double Lorene::Star_rot_diff::tsw ( ) const

virtual

Ratio T/W.

Reimplemented from Lorene::Star_rot.

Definition at line 41 of file strot_diff_global.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::b_car, Lorene::Star_rot::bbb, Lorene::Star::ener, Lorene::Star::ener_euler, Lorene::Star::gam_euler, Lorene::Scalar::integrale(), Lorene::Star::logn, Lorene::Star_rot::mass_g(), Lorene::Scalar::mult_rsint(), Lorene::Star::nbar, omega_field, Lorene::Star_rot::p_tsw, Lorene::Star::press, Lorene::Star_rot::relativistic, Lorene::Scalar::std_spectral_base(), and Lorene::Star_rot::uuu.

◆ update_metric()

void Lorene::Star_rot::update_metric ( )

inherited

Computes metric coefficients from known potentials.

The calculation is performed starting from the quantities logn , dzeta , tggg and shift , which are supposed to be up to date.
From these, the following fields are updated: nnn , a_car , bbb and b_car, as well as the 3-metric gamma.

Definition at line 54 of file star_rot_upmetr.C.

References Lorene::Star_rot::a_car, Lorene::Star_rot::b_car, Lorene::Star_rot::bbb, Lorene::Star_rot::del_deriv(), Lorene::Scalar::div_rsint(), Lorene::Star_rot::dzeta, Lorene::exp(), Lorene::Star_rot::extrinsic_curvature(), Lorene::Star::gamma, Lorene::Map::get_bvect_spher(), Lorene::Star::logn, Lorene::Star::mp, Lorene::Star::nn, Lorene::Tensor::set(), Lorene::Scalar::std_spectral_base(), Lorene::Star_rot::tggg, and Lorene::Star_rot::unsurc2.

◆ xi_surf()

const Tbl & Lorene::Star::xi_surf ( ) const

inherited

Description of the stellar surface: returns a 2-D Tbl containing the values of the radial coordinate $\xi$ on the surface at the collocation points in $(\theta', \phi')$ .

The stellar surface is defined as the location where the enthalpy (member ent) vanishes.

Definition at line 92 of file star_global.C.

References Lorene::Star::l_surf(), Lorene::Star::p_l_surf, and Lorene::Star::p_xi_surf.

◆ z_eqb()

double Lorene::Star_rot::z_eqb ( ) const

virtualinherited

Backward redshift factor at equator.

Definition at line 534 of file star_rot_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star_rot::p_z_eqb.

◆ z_eqf()

double Lorene::Star_rot::z_eqf ( ) const

virtualinherited

Forward redshift factor at equator.

Definition at line 506 of file star_rot_global.C.

References Lorene::Map::get_mg(), Lorene::Mg3d::get_type_t(), Lorene::Star::mp, and Lorene::Star_rot::p_z_eqf.

◆ z_pole()

double Lorene::Star_rot::z_pole ( ) const

virtualinherited

Redshift factor at North pole.

Definition at line 565 of file star_rot_global.C.

References Lorene::Star::nn, Lorene::Star_rot::p_z_pole, Lorene::Star::ray_pole(), and Lorene::Scalar::val_point().

Friends And Related Function Documentation

◆ operator<<

ostream& operator<<	(	ostream &	ost,
		const Star &	et
	)

friend

Display.

Definition at line 415 of file star.C.

Member Data Documentation

◆ a_car

Scalar Lorene::Star_rot::a_car

protectedinherited

Square of the metric factor A.

Definition at line 116 of file star_rot.h.

◆ ak_car

Scalar Lorene::Star_rot::ak_car

protectedinherited

Scalar $A^2 K_{ij} K^{ij}$ .

For axisymmetric stars, this quantity is related to the derivatives of $N^\varphi$ by

$A^2 K_{ij} K^{ij} = {B^2 \over 2 N^2} \, r^2\sin^2\theta \, \left[ \left( {\partial N^\varphi \over \partial r} \right) ^2 + {1\over r^2} \left( {\partial N^\varphi \over \partial \theta} \right) ^2 \right] \ .$

In particular it is related to the quantities $k_1$ and $k_2$ introduced by Eqs.~(3.7) and (3.8) of Bonazzola et al. Astron. Astrophys. 278 , 421 (1993) by

$A^2 K_{ij} K^{ij} = 2 A^2 (k_1^2 + k_2^2) \ .$

Definition at line 198 of file star_rot.h.

◆ b_car

Scalar Lorene::Star_rot::b_car

protectedinherited

Square of the metric factor B.

Definition at line 122 of file star_rot.h.

◆ bbb

Scalar Lorene::Star_rot::bbb

protectedinherited

Metric factor B.

Definition at line 119 of file star_rot.h.

◆ beta

Vector Lorene::Star::beta

protectedinherited

Shift vector.

Definition at line 228 of file star.h.

◆ dzeta

Scalar Lorene::Star_rot::dzeta

protectedinherited

Metric potential $\zeta = \ln(AN)$ .

Definition at line 146 of file star_rot.h.

◆ ener

Scalar Lorene::Star::ener

protectedinherited

Total energy density in the fluid frame.

Definition at line 193 of file star.h.

◆ ener_euler

Scalar Lorene::Star::ener_euler

protectedinherited

Total energy density in the Eulerian frame.

Definition at line 198 of file star.h.

◆ ent

Scalar Lorene::Star::ent

protectedinherited

Log-enthalpy.

Definition at line 190 of file star.h.

◆ eos

const Eos& Lorene::Star::eos

protectedinherited

Equation of state of the stellar matter.

Definition at line 185 of file star.h.

◆ gam_euler

Scalar Lorene::Star::gam_euler

protectedinherited

Lorentz factor between the fluid and Eulerian observers.

Definition at line 204 of file star.h.

◆ gamma

Metric Lorene::Star::gamma

protectedinherited

3-metric

Definition at line 235 of file star.h.

◆ khi_shift

Scalar Lorene::Star_rot::khi_shift

protectedinherited

Scalar $\chi$ used in the decomposition of shift , following Shibata's prescription [Prog.

Theor. Phys. 101 , 1199 (1999)] :

$N^i = {7\over 8} W^i - {1\over 8} \left(\nabla^i\chi+\nabla^iW^kx_k\right)$

Definition at line 172 of file star_rot.h.

◆ logn

Scalar Lorene::Star::logn

protectedinherited

Logarithm of the lapse N .

In the Newtonian case, this is the Newtonian gravitational potential (in units of $c^2$ ).

Definition at line 222 of file star.h.

◆ mp

Map& Lorene::Star::mp

protectedinherited

Mapping associated with the star.

Definition at line 180 of file star.h.

◆ nbar

Scalar Lorene::Star::nbar

protectedinherited

Baryon density in the fluid frame.

Definition at line 192 of file star.h.

◆ nn

Scalar Lorene::Star::nn

protectedinherited

Lapse function N .

Definition at line 225 of file star.h.

◆ nphi

Scalar Lorene::Star_rot::nphi

protectedinherited

Metric coefficient $N^\varphi$ .

Definition at line 125 of file star_rot.h.

◆ nuf

Scalar Lorene::Star_rot::nuf

protectedinherited

Part of the Metric potential $\nu = \ln N$ = logn generated by the matter terms.

Definition at line 138 of file star_rot.h.

◆ nuq

Scalar Lorene::Star_rot::nuq

protectedinherited

Part of the Metric potential $\nu = \ln N$ = logn generated by the quadratic terms.

Definition at line 143 of file star_rot.h.

◆ nzet

int Lorene::Star::nzet

protectedinherited

Number of domains of *mp occupied by the star.

Definition at line 183 of file star.h.

◆ omega

double Lorene::Star_rot::omega

protectedinherited

Rotation angular velocity ([f_unit] )

Definition at line 113 of file star_rot.h.

◆ omega_field

Scalar Lorene::Star_rot_diff::omega_field

protected

Field $\Omega(r,\theta)$ .

Definition at line 73 of file star_rot_diff.h.

◆ omega_frot

double(* Lorene::Star_rot_diff::omega_frot) (double, const Tbl &)

protected

Function $\Omega(F)$ defining the rotation profile.

The variable F is linked to the components of the fluid 4-velocity by

$F = u^t u_\varphi \ .$

The first argument of omega_frot must be $F$ ; the second argument contains the parameters, the first of which being necessarily the central value of $\Omega$ .

Definition at line 53 of file star_rot_diff.h.

◆ omega_max

double Lorene::Star_rot_diff::omega_max

protected

Maximum value of $\Omega$ .

Definition at line 76 of file star_rot_diff.h.

◆ omega_min

double Lorene::Star_rot_diff::omega_min

protected

Minimum value of $\Omega$ .

Definition at line 75 of file star_rot_diff.h.

◆ p_angu_mom

double* Lorene::Star_rot::p_angu_mom

mutableprotectedinherited

Angular momentum.

Definition at line 244 of file star_rot.h.

◆ p_aplat

double* Lorene::Star_rot::p_aplat

mutableprotectedinherited

Flatening r_pole/r_eq.

Definition at line 250 of file star_rot.h.

◆ p_area

double* Lorene::Star_rot::p_area

mutableprotectedinherited

Integrated surface area.

Definition at line 251 of file star_rot.h.

◆ p_espec_isco

double* Lorene::Star_rot::p_espec_isco

mutableprotectedinherited

Specific energy of a particle on the ISCO.

Definition at line 259 of file star_rot.h.

◆ p_f_eq

double* Lorene::Star_rot::p_f_eq

mutableprotectedinherited

Orbital frequency at the equator.

Definition at line 262 of file star_rot.h.

◆ p_f_isco

double* Lorene::Star_rot::p_f_isco

mutableprotectedinherited

Orbital frequency of the ISCO.

Definition at line 257 of file star_rot.h.

◆ p_grv2

double* Lorene::Star_rot::p_grv2

mutableprotectedinherited

Error on the virial identity GRV2.

Definition at line 246 of file star_rot.h.

◆ p_grv3

double* Lorene::Star_rot::p_grv3

mutableprotectedinherited

Error on the virial identity GRV3.

Definition at line 247 of file star_rot.h.

◆ p_l_surf

Itbl* Lorene::Star::p_l_surf

mutableprotectedinherited

Description of the stellar surface: 2-D Itbl containing the values of the domain index l on the surface at the collocation points in $(\theta', \phi')$ .

Definition at line 260 of file star.h.

◆ p_lspec_isco

double* Lorene::Star_rot::p_lspec_isco

mutableprotectedinherited

Specific angular momentum of a particle on the ISCO.

Definition at line 261 of file star_rot.h.

◆ p_mass_b

double* Lorene::Star::p_mass_b

mutableprotectedinherited

Baryon mass.

Definition at line 268 of file star.h.

◆ p_mass_g

double* Lorene::Star::p_mass_g

mutableprotectedinherited

Gravitational mass.

Definition at line 269 of file star.h.

◆ p_mom_quad

double* Lorene::Star_rot::p_mom_quad

mutableprotectedinherited

Quadrupole moment.

Definition at line 255 of file star_rot.h.

◆ p_r_circ

double* Lorene::Star_rot::p_r_circ

mutableprotectedinherited

Circumferential radius (equator)

Definition at line 248 of file star_rot.h.

◆ p_r_circ_merid

double* Lorene::Star_rot::p_r_circ_merid

mutableprotectedinherited

Circumferential radius (meridian)

Definition at line 249 of file star_rot.h.

◆ p_r_isco

double* Lorene::Star_rot::p_r_isco

mutableprotectedinherited

Circumferential radius of the ISCO.

Definition at line 256 of file star_rot.h.

◆ p_ray_eq

double* Lorene::Star::p_ray_eq

mutableprotectedinherited

Coordinate radius at $\phi=0$ , $\theta=\pi/2$ .

Definition at line 242 of file star.h.

◆ p_ray_eq_3pis2

double* Lorene::Star::p_ray_eq_3pis2

mutableprotectedinherited

Coordinate radius at $\phi=3\pi/2$ , $\theta=\pi/2$ .

Definition at line 251 of file star.h.

◆ p_ray_eq_pi

double* Lorene::Star::p_ray_eq_pi

mutableprotectedinherited

Coordinate radius at $\phi=\pi$ , $\theta=\pi/2$ .

Definition at line 248 of file star.h.

◆ p_ray_eq_pis2

double* Lorene::Star::p_ray_eq_pis2

mutableprotectedinherited

Coordinate radius at $\phi=\pi/2$ , $\theta=\pi/2$ .

Definition at line 245 of file star.h.

◆ p_ray_pole

double* Lorene::Star::p_ray_pole

mutableprotectedinherited

Coordinate radius at $\theta=0$ .

Definition at line 254 of file star.h.

◆ p_surf_grav

Tbl* Lorene::Star_rot::p_surf_grav

mutableprotectedinherited

Surface gravity (along the theta direction)

Definition at line 263 of file star_rot.h.

◆ p_tsw

double* Lorene::Star_rot::p_tsw

mutableprotectedinherited

Ratio T/W.

Definition at line 245 of file star_rot.h.

◆ p_xi_surf

Tbl* Lorene::Star::p_xi_surf

mutableprotectedinherited

Description of the stellar surface: 2-D Tbl containing the values of the radial coordinate $\xi$ on the surface at the collocation points in $(\theta', \phi')$ .

Definition at line 266 of file star.h.

◆ p_z_eqb

double* Lorene::Star_rot::p_z_eqb

mutableprotectedinherited

Backward redshift factor at equator.

Definition at line 253 of file star_rot.h.

◆ p_z_eqf

double* Lorene::Star_rot::p_z_eqf

mutableprotectedinherited

Forward redshift factor at equator.

Definition at line 252 of file star_rot.h.

◆ p_z_pole

double* Lorene::Star_rot::p_z_pole

mutableprotectedinherited

Redshift factor at North pole.

Definition at line 254 of file star_rot.h.

◆ par_frot

Tbl Lorene::Star_rot_diff::par_frot

protected

Parameters of the function $\Omega(F)$ .

To be used as the second argument of functions frot and primfrot . The parameter par_frot(0) must always be the central angular velocity.

Definition at line 70 of file star_rot_diff.h.

◆ press

Scalar Lorene::Star::press

protectedinherited

Fluid pressure.

Definition at line 194 of file star.h.

◆ prim_field

Scalar Lorene::Star_rot_diff::prim_field

protected

Field $\int_0^F F'\,\frac{d\Omega(F')}{dF'} \, dF'$ .

Definition at line 79 of file star_rot_diff.h.

◆ primfrot

double(* Lorene::Star_rot_diff::primfrot) (double, const Tbl &)

protected

Primitive of the function $F\frac{d\Omega(F)}{dF}$ , which vanishes at the stellar center.

The first argument of primfrot must be $F$ ; the second argument contains the parameters, the first of which being necessarily the central value of $\Omega$ .

Definition at line 61 of file star_rot_diff.h.

◆ relativistic

bool Lorene::Star_rot::relativistic

protectedinherited

Indicator of relativity: true for a relativistic star, false for a Newtonian one.

Definition at line 106 of file star_rot.h.

◆ s_euler

Scalar Lorene::Star::s_euler

protectedinherited

Trace of the stress scalar in the Eulerian frame.

Definition at line 201 of file star.h.

◆ ssjm1_dzeta

Scalar Lorene::Star_rot::ssjm1_dzeta

protectedinherited

Effective source at the previous step for the resolution of the Poisson equation for dzeta .

Definition at line 215 of file star_rot.h.

◆ ssjm1_khi

Scalar Lorene::Star_rot::ssjm1_khi

protectedinherited

Effective source at the previous step for the resolution of the Poisson equation for the scalar $\chi$ by means of Map_et::poisson .

$\chi$ is an intermediate quantity for the resolution of the elliptic equation for the shift vector $N^i$

Definition at line 228 of file star_rot.h.

◆ ssjm1_nuf

Scalar Lorene::Star_rot::ssjm1_nuf

protectedinherited

Effective source at the previous step for the resolution of the Poisson equation for nuf by means of Map_et::poisson .

Definition at line 204 of file star_rot.h.

◆ ssjm1_nuq

Scalar Lorene::Star_rot::ssjm1_nuq

protectedinherited

Effective source at the previous step for the resolution of the Poisson equation for nuq by means of Map_et::poisson .

Definition at line 210 of file star_rot.h.

◆ ssjm1_tggg

Scalar Lorene::Star_rot::ssjm1_tggg

protectedinherited

Effective source at the previous step for the resolution of the Poisson equation for tggg .

Definition at line 220 of file star_rot.h.

◆ ssjm1_wshift

Vector Lorene::Star_rot::ssjm1_wshift

protectedinherited

Effective source at the previous step for the resolution of the vector Poisson equation for $W^i$ .

$W^i$ is an intermediate quantity for the resolution of the elliptic equation for the shift vector $N^i$ (Components with respect to the Cartesian triad associated with the mapping mp )

Definition at line 237 of file star_rot.h.

◆ stress_euler

Sym_tensor Lorene::Star::stress_euler

protectedinherited

Spatial part of the stress-energy tensor with respect to the Eulerian observer.

Definition at line 212 of file star.h.

◆ tggg

Scalar Lorene::Star_rot::tggg

protectedinherited

Metric potential $\tilde G = (NB-1) r\sin\theta$ .

Definition at line 149 of file star_rot.h.

◆ tkij

Sym_tensor Lorene::Star_rot::tkij

protectedinherited

Tensor ${\tilde K_{ij}}$ related to the extrinsic curvature tensor by ${\tilde K_{ij}} = B^{-2} K_{ij}$ .

tkij contains the Cartesian components of ${\tilde K_{ij}}$ .

Definition at line 179 of file star_rot.h.

◆ tnphi

Scalar Lorene::Star_rot::tnphi

protectedinherited

Component $\tilde N^\varphi = N^\varphi r\sin\theta$ of the shift vector.

Definition at line 130 of file star_rot.h.

◆ u_euler

Vector Lorene::Star::u_euler

protectedinherited

Fluid 3-velocity with respect to the Eulerian observer.

Definition at line 207 of file star.h.

◆ unsurc2

double Lorene::Star_rot::unsurc2

protectedinherited

$1/c^2$ : unsurc2=1 for a relativistic star, 0 for a Newtonian one.

Definition at line 111 of file star_rot.h.

◆ uuu

Scalar Lorene::Star_rot::uuu

protectedinherited

Norm of u_euler.

Definition at line 133 of file star_rot.h.

◆ w_shift

Vector Lorene::Star_rot::w_shift

protectedinherited

Vector $W^i$ used in the decomposition of shift , following Shibata's prescription [Prog.

Theor. Phys. 101 , 1199 (1999)] :

$N^i = {7\over 8} W^i - {1\over 8} \left(\nabla^i\chi+\nabla^iW^kx_k\right)$

NB: w_shift contains the components of $W^i$ with respect to the Cartesian triad associated with the mapping mp .

Definition at line 162 of file star_rot.h.

The documentation for this class was generated from the following files:

Public Member Functions

Static Public Member Functions

Protected Member Functions

Protected Attributes

Friends

Detailed Description

Constructor & Destructor Documentation

◆ Star_rot_diff() [1/3]

◆ Star_rot_diff() [2/3]

◆ Star_rot_diff() [3/3]

◆ ~Star_rot_diff()

Member Function Documentation

◆ angu_mom()

◆ aplat()

◆ area()

◆ del_deriv()

◆ del_hydro_euler()

◆ display_poly()

◆ equation_of_state()

◆ equilibrium()

◆ equilibrium_spher()

◆ espec_isco()

◆ extrinsic_curvature()

◆ f_eq()

◆ f_isco()

◆ fait_nphi()

◆ fait_omega_field()

◆ fait_prim_field()

◆ fait_shift()

◆ get_a_car()

◆ get_ak_car()

◆ get_b_car()

◆ get_bbb()

◆ get_beta()

◆ get_dzeta()

◆ get_ener()

◆ get_ener_euler()

◆ get_ent()

◆ get_eos()

◆ get_gam_euler()

◆ get_gamma()

◆ get_khi_shift()

◆ get_logn()

◆ get_mp()

◆ get_nbar()

◆ get_nn()

◆ get_nphi()

◆ get_nuf()

◆ get_nuq()

◆ get_nzet()

◆ get_omega_c()

◆ get_omega_field()

◆ get_press()

◆ get_s_euler()

◆ get_stress_euler()

◆ get_tggg()

◆ get_tkij()

◆ get_tnphi()

◆ get_u_euler()

◆ get_uuu()

◆ get_w_shift()

◆ grv2()

◆ grv3()

◆ hydro_euler()

◆ is_relativistic()

◆ l_surf()

◆ lambda_grv2()

◆ lspec_isco()

◆ mass_b()

◆ mass_g()

◆ mean_radius()

◆ mom_quad()

◆ omega_funct()

◆ operator=()

◆ operator>>()

◆ partial_display()

◆ prim_funct_omega()

◆ r_circ()

◆ r_circ_merid()

◆ r_isco()