This MODULE contains the definition of TYPE bnsbase, which is an ABSTRACT TYPE representing any possible type of binary neutron star (\(\mathrm{BNS}\)) initial data (\(\mathrm{ID}\)) to be set up for \(\texttt{SPHINCS_BSSN}\). That is, \(\mathrm{BNS}\) \(\mathrm{ID}\) produced with \(\texttt{LORENE}\), with \(\texttt{FUKA}\), etc.
PROCEDURES and variables shared by all the types of \(\mathrm{BNS}\) \(\mathrm{ID}\) should belong to TYPE bnsbase, as they are inherited by its EXTENDED TYPES that represent more specific types of \(\mathrm{BNS}\) \(\mathrm{ID}\).
FT 24.09.2021
Finds the center of a star, as the point where the density is maximal.
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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double precision, | intent(in) | :: | separation |
Separation between the stars |
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double precision, | intent(in) | :: | x_sign |
Sign of the x coordinates of the point inside the star |
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procedure(get_density_at_pos), | optional | :: | get_density |
Center of a star, as the point where the density is maximal.
Finds the radius of a matter object, relative to a center and along a direction. The radius is determined as the first point where the density is zero.
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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double precision, | intent(in), | DIMENSION(3) | :: | center |
Center point relative to which the radius is measured |
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double precision, | intent(in), | DIMENSION(3) | :: | vector |
Vector that defines the direction along which to measure the radius. If not normalized, it will be normalized. |
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procedure(get_density_at_pos), | optional | :: | get_density |
Radius of the star relative to center
, along the direction
specified by vector
Finds the surface of a star, using [[bnsbase::find_radius]] along many directions.
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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double precision, | intent(in), | DIMENSION(3) | :: | center |
Center point relative to which the radius is measured |
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integer, | intent(in) | :: | n_theta |
Number of points in for the colatitude |
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integer, | intent(in) | :: | n_phi |
Number of points in for the azimuth |
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double precision, | intent(out), | DIMENSION(:,:,:), ALLOCATABLE | :: | surface |
Array storing the coordinates of the points on the surface |
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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integer, | intent(in) | :: | i_matter |
Index of the matter object whose parameter is to return |
Result
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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integer, | intent(in) | :: | i_matter |
Index of the matter object whose parameter is to return |
Result
Type | Intent | Optional | Attributes | Name | ||
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class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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integer, | intent(in) | :: | i_matter |
Index of the matter object whose string is to return |
Result
Prints a summary of the physical properties the \(\mathrm{BNS}\) system
to the standard output and, optionally, to a formatted file whose name
is given as the optional argument filename
Type | Intent | Optional | Attributes | Name | ||
---|---|---|---|---|---|---|
class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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character(len=*), | intent(inout), | optional | :: | filename |
Name of the formatted file to print the summary to |
Prints a summary of the physical properties the system
to the standard output and, optionally, to a formatted file whose name
is given as the optional argument filename
Type | Intent | Optional | Attributes | Name | ||
---|---|---|---|---|---|---|
class(bnsbase), | intent(in) | :: | this |
bnsbase object owning this PROCEDURE |
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character(len=*), | intent(inout), | optional | :: | filename |
Name of the formatted file to print the summary to |
ABSTRACT TYPE for \(\mathrm{BNS}\) \(\mathrm{ID}\) (produced with \(\texttt{LORENE}\), or with \(\texttt{FUKA}\), etc.; or produced with the same tool, but read in different ways, for example by linking to the \(\texttt{LORENE}\) library, or reading the \(\mathrm{ID}\) from a lattice, etc.)
Type | Visibility | Attributes | Name | Initial | |||
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double precision, | public | :: | adm_mass |
ADM mass of the system |
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double precision, | public | :: | angular_momentum_x | = | 0.0D0 |
component of the angular momentum of the BNS system |
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double precision, | public | :: | angular_momentum_y | = | 0.0D0 |
component of the angular momentum of the BNS system |
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double precision, | public | :: | angular_momentum_z | = | 0.0D0 |
component of the angular momentum of the BNS system |
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double precision, | public | :: | angular_vel |
Angular velocity |
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double precision, | public | :: | area_radius1 |
Areal (or circumferential) radius of star 1 Note that these is the areal radius of the star in the binary system, which is different than that of an isolated star. The latter is used in the mass-radius diagrams, together with the gravitatonal mass |
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double precision, | public | :: | area_radius2 |
Areal (or circumferential) radius of star 2 Note that these is the areal radius of the star in the binary system, which is different than that of an isolated star. The latter is used in the mass-radius diagrams, together with the gravitatonal mass |
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double precision, | public, | DIMENSION(2,3) | :: | barycenter |
Array containing the barycenters of the stars |
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double precision, | public | :: | barycenter1_x |
Barycenter of star 1 |
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double precision, | public | :: | barycenter2_x |
Barycenter of star 2 |
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double precision, | public, | DIMENSION(3) | :: | barycenter_system |
Array containing the barycenters of the stars |
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double precision, | public, | DIMENSION(2,3) | :: | center |
Array containing the centers of the stars |
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double precision, | public | :: | center1_x |
Stellar center of star 1 (origin of the LORENE chart centered on star 1) |
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double precision, | public | :: | center2_x |
Stellar center of star 2 (origin of the LORENE chart centered on star 2) |
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type(timer), | public | :: | construction_timer |
Timer that times the construction of the appropriate object |
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double precision, | public | :: | distance |
Distance between the points of maximum baryon density |
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double precision, | public | :: | distance_com |
Distance between the centers of mass |
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double precision, | public | :: | energy_density_center1 |
Central energy density for star 1 |
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double precision, | public | :: | energy_density_center2 |
Central energy density for star 2 |
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double precision, | public | :: | ent_center1 |
Central enthalpy for star 1 |
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double precision, | public | :: | ent_center2 |
Central enthalpy for star 2 |
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character(len=:), | public, | ALLOCATABLE | :: | eos1 |
Name of the equation of state (\(\mathrm{EOS}\)) of star 1 |
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integer, | public | :: | eos1_id |
\(\texttt{SPHINCS_ID}\) identifier for the \(\mathrm{EOS}\) of star 1 |
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character(len=:), | public, | ALLOCATABLE | :: | eos2 |
Name of the equation of state (\(\mathrm{EOS}\)) of star 2 |
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integer, | public | :: | eos2_id |
\(\texttt{SPHINCS_ID}\) identifier for the \(\mathrm{EOS}\) of star 2 |
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character(len=max_length), | public, | DIMENSION(2) | :: | eos_filenames |
Array of strings containing the names of the files containing the \(\mathrm{EOS}\) to be used for each matter object. |
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character(len=:), | public, | ALLOCATABLE | :: | eos_table1 |
String containing the path to the files containing the table of the \(\mathrm{EOS}\) for star 1. |
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character(len=:), | public, | ALLOCATABLE | :: | eos_table2 |
String containing the path to the files containing the table of the \(\mathrm{EOS}\) for star 2. |
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procedure, | public, | POINTER, NOPASS | :: | finalize_sph_id_ptr |
Pointer to a procedure that finalize the \(\mathrm{SPH}\) \(\mathrm{ID}\); for example, correct for the residual ADM linear momentum. |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_xx |
1-D array storing the xx component of the spatial metric [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_xy |
1-D array storing the xy component of the spatial metric [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_xz |
1-D array storing the xz component of the spatial metric [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_yy |
1-D array storing the yy component of the spatial metric [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_yz |
1-D array storing the yz component of the spatial metric [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | g_zz |
1-D array storing the zz component of the spatial metric [pure number] |
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double precision, | public | :: | gamma0_1 |
Piecewise polytrope: polytropic index for star 1 |
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double precision, | public | :: | gamma0_2 |
Piecewise polytrope: polytropic index for star 2 |
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double precision, | public | :: | gamma1_1 |
Piecewise polytrope: polytropic index for star 1 |
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double precision, | public | :: | gamma1_2 |
Piecewise polytrope: polytropic index for star 2 |
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double precision, | public | :: | gamma2_1 |
Piecewise polytrope: polytropic index for star 1 |
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double precision, | public | :: | gamma2_2 |
Piecewise polytrope: polytropic index for star 2 |
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double precision, | public | :: | gamma3_1 |
Piecewise polytrope: polytropic index for star 1 |
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double precision, | public | :: | gamma3_2 |
Piecewise polytrope: polytropic index for star 2 |
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double precision, | public | :: | gamma_1 |
Single polytrope: polytropic index for star 1 |
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double precision, | public | :: | gamma_2 |
Single polytrope: polytropic index for star 2 |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_xx |
1-D array storing the xx component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_xy |
1-D array storing the xy component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_xz |
1-D array storing the xz component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_yy |
1-D array storing the yy component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_yz |
1-D array storing the yz component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | k_zz |
1-D array storing the zz component of the extrinsic curvature [c/MSun_geo] |
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double precision, | public | :: | kappa0_1 |
Piecewise polytrope: polytropic constant for star 1 [pure number] |
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double precision, | public | :: | kappa0_2 |
Piecewise polytrope: polytropic constant for star 2 [pure number] |
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double precision, | public | :: | kappa1_1 |
Piecewise polytrope: polytropic constant for star 1 [pure number] |
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double precision, | public | :: | kappa1_2 |
Piecewise polytrope: polytropic constant for star 2 [pure number] |
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double precision, | public | :: | kappa2_1 |
Piecewise polytrope: polytropic constant for star 1 [pure number] |
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double precision, | public | :: | kappa2_2 |
Piecewise polytrope: polytropic constant for star 2 [pure number] |
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double precision, | public | :: | kappa3_1 |
Piecewise polytrope: polytropic constant for star 1 [pure number] |
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double precision, | public | :: | kappa3_2 |
Piecewise polytrope: polytropic constant for star 2 [pure number] |
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double precision, | public | :: | kappa_1 |
Single polytrope: polytropic constant for star 1 [pure number] |
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double precision, | public | :: | kappa_2 |
Single polytrope: polytropic constant for star 2 [pure number] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | lapse |
1-D array storing the lapse function |
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double precision, | public | :: | linear_momentum_x | = | 0.0D0 |
component of the ADM linear momentum of the system |
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double precision, | public | :: | linear_momentum_y | = | 0.0D0 |
component of the ADM linear momentum of the system |
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double precision, | public | :: | linear_momentum_z | = | 0.0D0 |
component of the ADM linear momentum of the system |
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double precision, | public | :: | logP1_1 |
Piecewise polytrope: Base 10 exponent of the pressure at the first fiducial density (between and ) for star 1 |
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double precision, | public | :: | logP1_2 |
Piecewise polytrope: Base 10 exponent of the pressure at the first fiducial density (between and ) for star 2 |
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double precision, | public | :: | logRho0_1 |
Piecewise polytrope: Base 10 exponent of the first fiducial density (between and ) for star 1 |
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double precision, | public | :: | logRho0_2 |
Piecewise polytrope: Base 10 exponent of the second fiducial density (between and ) for star 2 |
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double precision, | public | :: | logRho1_1 |
Piecewise polytrope: Base 10 exponent of the second fiducial density (between and ) for star 1 |
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double precision, | public | :: | logRho1_2 |
Piecewise polytrope: Base 10 exponent of the second fiducial density (between and ) for star 2 |
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double precision, | public | :: | logRho2_1 |
Piecewise polytrope: Base 10 exponent of the third fiducial density (between and ) for star 1 |
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double precision, | public | :: | logRho2_2 |
Piecewise polytrope: Base 10 exponent of the third fiducial density (between and ) for star 2 |
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double precision, | public | :: | mOmega |
mOmega= ( angular_vel ) ( mass_grav1 + mass_grav2 ) [pure number] |
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double precision, | public, | DIMENSION(2) | :: | mass |
Array containing the baryonic masses |
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double precision, | public | :: | mass1 |
Baryonic mass of star 1 |
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double precision, | public | :: | mass2 |
Baryonic mass of star 2 |
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double precision, | public, | DIMENSION(2) | :: | mass_grav |
Array containing the gravitational masses |
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double precision, | public | :: | mass_grav1 |
Gravitational mass of star 1 |
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double precision, | public | :: | mass_grav2 |
Gravitational mass of star 2 |
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double precision, | public | :: | nbar_center1 |
Central baryon number density for star 1 |
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double precision, | public | :: | nbar_center2 |
Central baryon number density for star 2 |
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integer, | public | :: | npeos_1 |
Piecewise polytrope: Number of polytropic pieces for star 1 |
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integer, | public | :: | npeos_2 |
Piecewise polytrope: Number of polytropic pieces for star 2 |
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double precision, | public | :: | pressure_center1 |
Central pressure for star 1 |
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double precision, | public | :: | pressure_center2 |
Central pressure for star 2 |
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double precision, | public, | DIMENSION(2,6) | :: | radii |
Array containing the signed radii of the stars |
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double precision, | public | :: | radius1_x_comp |
Radius of star 1, in the x direction, towards the companion |
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double precision, | public | :: | radius1_x_opp |
Radius of star 1, in the x direction, opposite to companion |
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double precision, | public | :: | radius1_y |
Radius of star 1, in the y direction |
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double precision, | public | :: | radius1_z |
Radius of star 1, in the z direction |
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double precision, | public | :: | radius2_x_comp |
Radius of star 2, in the x direction, towards the companion |
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double precision, | public | :: | radius2_x_opp |
Radius of star 2, in the x direction, opposite to companion |
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double precision, | public | :: | radius2_y |
Radius of star 2, in the y direction |
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double precision, | public | :: | radius2_z |
Radius of star 2, in the z direction |
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double precision, | public | :: | rho_center1 |
Central baryon mass density for star 1 |
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double precision, | public | :: | rho_center2 |
Central baryon mass density for star 2 |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | shift_x |
1-D array storing the x component of the shift vector [c] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | shift_y |
1-D array storing the y component of the shift vector [c] |
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double precision, | public, | DIMENSION(:), ALLOCATABLE | :: | shift_z |
1-D array storing the z component of the shift vector [c] |
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double precision, | public | :: | specific_energy_center1 |
Central specific energy for star 1 |
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double precision, | public | :: | specific_energy_center2 |
Central specific energy for star 2 |
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type(surface), | public, | DIMENSION(:), ALLOCATABLE | :: | surfaces |
Array containing, for each matter object, a set of coordinates of some points modelling the surfaces. |
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double precision, | public | :: | t_merger |
Estimated time of the merger P. C. Peters, "Gravitational Radiation and the Motion of Two Point Masses", Phys. Rev. 136, B1224 (1964) |
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type(tabu_eos), | public, | DIMENSION(:), ALLOCATABLE | :: | tab_eos |
Array containing a tabulated \(\mathrm{EOS}\) for each matter object, when used. |
procedure , public , NON_OVERRIDABLE :: check_i_matter Interface | Checks that the given index is between 1 and n_matter, included. If not, it stops the execution of the program. |
procedure (derived_type_constructor_int) , public :: derived_type_constructor | Constructs a TYPE that extends idbase |
procedure , public :: estimate_lengthscale_field Interface | Estimate typical length scales, one per each matter object, by computing , where is a field given as input, and represent a derivative of it. Presently, the derivatives are computed separately along each spatial dimension, as 1D derivatives. |
procedure , public , NON_OVERRIDABLE :: find_center Interface | Finds the center of a matter object, as the point where the density is maximal. |
procedure , public , NON_OVERRIDABLE :: find_print_surfaces Interface | Finds the surfaces of the stars, and prints them to a formatted file. |
procedure , public , NON_OVERRIDABLE :: find_radius Interface | Finds the radius of a star, relative to a center and along a direction. The radius is determined as the first point where the density is zero. |
procedure , public , NON_OVERRIDABLE :: find_surface Interface | Finds the surface of a star, using [[bnsbase::find_radius]] along many directions. |
procedure , public :: get_adm_mass Interface | Returns adm_mass |
procedure , public :: get_angular_momentum Interface | Returns the angular momentum vector angular_momentum_x, angular_momentum_y, angular_momentum_z |
procedure , public :: get_angular_vel Interface | Returns angular_vel |
procedure , public :: get_barycenter1_x Interface | Returns barycenter1_x |
procedure , public :: get_barycenter2_x Interface | Returns barycenter2_x |
procedure , public :: get_center1_x Interface | Returns center1_x |
procedure , public :: get_center2_x Interface | Returns center2_x |
procedure , public , NON_OVERRIDABLE :: get_cold_system Interface | Returns cold_system, the |
procedure , public :: get_distance Interface | Returns distance |
procedure , public :: get_distance_com Interface | Returns distance_com |
procedure , public :: get_energy_density_center1 Interface | Returns energy_density_center1 |
procedure , public :: get_energy_density_center2 Interface | Returns energy_density_center2 |
procedure , public :: get_ent_center1 Interface | Returns ent_center1 |
procedure , public :: get_ent_center2 Interface | Returns ent_center2 |
procedure , public :: get_eos1 Interface | Returns eos1 |
procedure (get_eos_id_int) , public :: get_eos1_id | Returns an integer that identifies the equation of state of star 1 |
procedure , public :: get_eos2 Interface | Returns eos2 |
procedure (get_eos_id_int) , public :: get_eos2_id | Returns an integer that identifies the equation of state of star 2 |
procedure , public :: get_eos_id Interface | |
procedure , public , NON_OVERRIDABLE :: get_estimate_length_scale Interface | Returns estimate_length_scale, the |
procedure , public :: get_gamma0_1 Interface | Returns gamma0_1 |
procedure , public :: get_gamma0_2 Interface | Returns gamma0_2 |
procedure , public :: get_gamma1_1 Interface | Returns gamma1_1 |
procedure , public :: get_gamma1_2 Interface | Returns gamma1_2 |
procedure , public :: get_gamma2_1 Interface | Returns gamma2_1 |
procedure , public :: get_gamma2_2 Interface | Returns gamma2_2 |
procedure , public :: get_gamma3_1 Interface | Returns gamma3_1 |
procedure , public :: get_gamma3_2 Interface | Returns gamma3_2 |
procedure , public :: get_gamma_1 Interface | Returns gamma_1 |
procedure , public :: get_gamma_2 Interface | Returns gamma_2 |
procedure , public :: get_grav_mass1 Interface | Returns mass_grav1 |
procedure , public :: get_grav_mass2 Interface | Returns mass_grav2 |
procedure , public :: get_kappa0_1 Interface | Returns kappa0_1 |
procedure , public :: get_kappa0_2 Interface | Returns kappa0_2 |
procedure , public :: get_kappa1_1 Interface | Returns kappa1_1 |
procedure , public :: get_kappa1_2 Interface | Returns kappa1_2 |
procedure , public :: get_kappa2_1 Interface | Returns kappa2_1 |
procedure , public :: get_kappa2_2 Interface | Returns kappa2_2 |
procedure , public :: get_kappa3_1 Interface | Returns kappa3_1 |
procedure , public :: get_kappa3_2 Interface | Returns kappa3_2 |
procedure , public :: get_kappa_1 Interface | Returns kappa_1 |
procedure , public :: get_kappa_2 Interface | Returns kappa_2 |
procedure , public :: get_linear_momentum Interface | Returns the linear momentum vector linear_momentum_x, linear_momentum_y, linear_momentum_z |
procedure , public :: get_logP1_1 Interface | Returns logP1_1 |
procedure , public :: get_logP1_2 Interface | Returns logP1_2 |
procedure , public :: get_logRho0_1 Interface | Returns logRho0_1 |
procedure , public :: get_logRho0_2 Interface | Returns logRho0_2 |
procedure , public :: get_logRho1_1 Interface | Returns logRho1_1 |
procedure , public :: get_logRho1_2 Interface | Returns logRho1_2 |
procedure , public :: get_logRho2_1 Interface | Returns logRho2_1 |
procedure , public :: get_logRho2_2 Interface | Returns logRho2_2 |
procedure , public :: get_mass1 Interface | Returns mass1 |
procedure , public :: get_mass2 Interface | Returns mass2 |
procedure , public , NON_OVERRIDABLE :: get_n_matter Interface | Returns n_matter, the number of matter objects in the physical system |
procedure , public :: get_nbar_center1 Interface | Returns nbar_center1 |
procedure , public :: get_nbar_center2 Interface | Returns nbar_center2 |
procedure , public :: get_npeos_1 Interface | Returns npeos_1 |
procedure , public :: get_npeos_2 Interface | Returns npeos_2 |
procedure , public , NON_OVERRIDABLE :: get_one_lapse Interface | Returns one_lapse, the |
procedure , public :: get_pressure_center1 Interface | Returns pressure_center1 |
procedure , public :: get_pressure_center2 Interface | Returns pressure_center2 |
procedure , public :: get_radius1_x_comp Interface | Returns radius1_x_comp |
procedure , public :: get_radius1_x_opp Interface | Returns radius1_x_opp |
procedure , public :: get_radius1_y Interface | Returns radius1_y |
procedure , public :: get_radius1_z Interface | Returns radius1_z |
procedure , public :: get_radius2_x_comp Interface | Returns radius2_x_comp |
procedure , public :: get_radius2_x_opp Interface | Returns radius2_x_opp |
procedure , public :: get_radius2_y Interface | Returns radius2_y |
procedure , public :: get_radius2_z Interface | Returns radius2_y |
procedure , public :: get_rho_center1 Interface | Returns rho_center1 |
procedure , public :: get_rho_center2 Interface | Returns rho_center2 |
procedure , public :: get_specific_energy_center1 Interface | Returns specific_energy_center1 |
procedure , public :: get_specific_energy_center2 Interface | Returns specific_energy_center2 |
procedure , public , NON_OVERRIDABLE :: get_total_spatial_extent Interface | Returns the spatial extent of the physical system considered, as the array of 6 numbers |
procedure , public , NON_OVERRIDABLE :: get_zero_shift Interface | Returns zero_shift, the |
procedure , public , NON_OVERRIDABLE :: initialize Interface | This PROCEDURE calls the constructor of the idbase-extended type and the SUBROUTINE sanity_check afterwards. It is recommended to use this SUBROUTINE to construct objects of idbase-extended type since the sanity check is performed automatically. |
procedure (initialize_id_int) , public :: initialize_id | Initialize the \(\mathrm{ID}\); for example, set up the lattices around the stars for the \(\mathrm{BNS}\) produced with \(\texttt{FUKA}\). |
procedure , public :: integrate_baryon_mass_density Interface | Integrates the baryon mass density over a matter object, using spherical coordinates, and computes its radial profile inside the star |
procedure , public :: print_summary => print_summary_bnsbase Interface | |
procedure (print_summary_derived_int) , public :: print_summary_derived | Prints a summary of the physical properties the system to the standard output and, optionally, to a formatted file whose name is given as optional argument. Printse information relative to the derived type oly |
procedure (read_id_full_int) , public :: read_id_full | Reads the full \(\mathrm{ID}\) |
procedure (read_id_hydro_int) , public :: read_id_hydro | Reads the hydro \(\mathrm{ID}\) needed to compute the constraints on the refined mesh |
procedure (read_id_k_int) , public :: read_id_k | Reads the components of the extrinsic curvature |
procedure (read_id_mass_b_int) , public :: read_id_mass_b | Reads the hydro \(\mathrm{ID}\) needed to compute the baryon mass |
procedure (read_id_particles_int) , public :: read_id_particles | Reads the hydro \(\mathrm{ID}\) needed to compute the SPH \(\mathrm{ID}\) |
procedure (read_id_spacetime_int) , public :: read_id_spacetime | Reads the spacetime \(\mathrm{ID}\) needed to compute the BSSN variables and constraints |
procedure (read_double_at_pos) , public :: read_mass_density | Returns the baryon mass density from the \(\mathrm{ID}\) at the given point |
procedure (read_double_at_pos) , public :: read_pressure | Returns the pressure from te \(\mathrm{ID}\) at the given point |
procedure , public :: return_adm_mass => get_adm_mass Interface | |
procedure , public :: return_barycenter => get_barycenter Interface | |
procedure , public :: return_center => get_center Interface | |
procedure , public :: return_eos_name => get_eos Interface | |
procedure (return_eos_parameters_int) , public :: return_eos_parameters | Returns the identification number of the \(\mathrm{EOS}\) of the matter objects. |
procedure , public :: return_mass => get_mass Interface | |
procedure , public :: return_spatial_extent => get_radii Interface | |
procedure , public , NON_OVERRIDABLE :: sanity_check Interface | Checks that n_matter and the sizes returned by return_spatial_extent and get_total_spatial_extent are acceptable. It is called by initialize, after the constructor of the derived type. |
procedure , public , NON_OVERRIDABLE :: set_cold_system Interface | Sets cold_system, the |
procedure , public , NON_OVERRIDABLE :: set_estimate_length_scale Interface | Sets estimate_length_scale, the |
procedure , public , NON_OVERRIDABLE :: set_n_matter Interface | Sets n_matter, the number of matter objects in the physical system, to a value |
procedure , public , NON_OVERRIDABLE :: set_one_lapse Interface | Sets one_lapse, the |
procedure , public , NON_OVERRIDABLE :: set_zero_shift Interface | Sets zero_shift, the |
procedure (read_logical_at_pos) , public :: test_position | Returns |