read Submodule

Return 1 if the energy density is nonpositive or if the specific energy is nonpositive, or if the pressure is nonpositive at the specified point

Arguments

Return Value logical

.TRUE. if the energy density or the specific energy or the pressure are negative, .FALSE. otherwise

Stores the \(\mathrm{ID}\) in non-bnsfuka-member arrays with the same shape as the bnsfuka member arrays

Arguments

Stores the hydro \(\mathrm{ID}\) in the arrays needed to compute the constraints on the refined mesh

Arguments

Stores the components of the extrinsic curvature in arrays

Arguments

Stores the hydro \(\mathrm{ID}\) in the arrays needed to compute the baryon mass, storing it to variables (not arrays as the others SUBROUTINES in this SUBMODULE).

Arguments

Stores the \(\mathrm{ID}\) in the bnsfuka member arrays

Arguments

Stores the hydro \(\mathrm{ID}\) in the arrays needed to compute the \(\mathrm{SPH}\) \(\mathrm{ID}\)

Arguments

Stores the spacetime \(\mathrm{ID}\) in multi-dimensional arrays needed to compute the BSSN variables and constraints

Arguments

Returns the \(\texttt{FUKA}\) mass density at the point given as argument, in units of $M_\odot/\ell_\odot^3$.

Arguments

Return Value double precision

Baryon mass density at $(x,y,z)$

Returns the \(\texttt{FUKA}\) pressure at the point given as argument, in units of $M_\odot c^2/\ell_\odot^3$.

Arguments

Return Value double precision

Pressure at $(x,y,z)$

Returns the \(\texttt{FUKA}\) conformal factor to the 4th power, equal to the diagonal components of the conformally flat spatial ADM metric.

Arguments

Return Value real(kind=C_DOUBLE)

$g_{xx}=g_{yy}=g_{zz}$ at $(x,y,z)$

Calls the MPI-parallelized version of the function KadathExportBNS within Kadath

Arguments

Read the \(\texttt{FUKA}\) \(\mathrm{ID}\) on two lattices, each one enclosing a star. The lattices are needed to interpolate the \(\mathrm{ID}\) on the particles.

Arguments