Binary neutron star configuration on a Cartesian grid.
Binary neutron star configuration on a Cartesian grid.A binary black hole system is constructed on a Cartesian grid from data stored in a file resulting from a computation by Taniguchi and Gourgoulhon.
Importation of Lorene data is performed by means of the constructor Bin_NS::Bin_NS(int, const double*, const double*, const double*, const char*). This constructor takes general arrays for the location of the Cartesian coordinates
, i.e. it does not assume that the grid is a uniform one. Note also that these arrays are 1-D, as well as all the metric fields, in order to be use with any ordering of the 3-D storage.
This class is very simple, with all data members being public. A typical example of use is the following one
* // Define the Cartesian grid by means of the arrays xg, yg, zg: * for (int i=0; i<nb_points; i++) { * xg[i] = ... * yg[i] = ... * zg[i] = ... * } * * // Read the file containing the spectral data and evaluate * // all the fields on the Cartesian grid : * * Bin_NS binary_system(nb_points, xg, yg, zg, datafile) ; * * // Extract what you need : * * double* gamma_xx = binary_system.g_xx ; // metric coefficient g_xx * * double* shift_x = binary_system.beta_x ; // x comp. of shift vector * * ... * * // Save everything in an ASCII file : * * ofstream file_ini("ini.d") ; * binary_system.save_form(file_ini) ; * file_ini.close() ; * *
]
]
]
]
]
]
at the np grid points (1-D array)
of the shift vector of non rotating coordinates [unit:
]
of the shift vector of non rotating coordinates [unit:
]
of the shift vector of non rotating coordinates [unit:
]
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
]
]
of the fluid 3-velocity with respect to the Eulerian observer, at the np grid points (1-D array) [unit:
]
of the fluid 3-velocity with respect to the Eulerian observer, at the np grid points (1-D array) [unit:
]
of the fluid 3-velocity with respect to the Eulerian observer, at the np grid points (1-D array) [unit:
]
]
]
]
]
]
]
at the np grid points (1-D array)
of the shift vector of non rotating coordinates [unit:
]
of the shift vector of non rotating coordinates [unit:
]
of the shift vector of non rotating coordinates [unit:
]
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
at the grid points (1-D array)
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
of the extrinsic curvature at the grid points (1-D array) [unit: c/km]
]
]
of the fluid 3-velocity with respect to the Eulerian
observer, at the np grid points (1-D array) [unit:
]
of the fluid 3-velocity with respect to the Eulerian
observer, at the np grid points (1-D array) [unit:
]
of the fluid 3-velocity with respect to the Eulerian
observer, at the np grid points (1-D array) [unit:
]
This constructor takes general arrays xi, yi, zi
for the location of the Cartesian coordinates
, i.e. it does not assume that the grid is a uniform one.
These arrays are 1-D to deal with any ordering of a 3-D storage.
Index alphabétique Hiérarchie des classes HTML ou Java