interpolate Submodule

Stores the \(\mathrm{ID}\) in non-ejecta-member arrays with the same shape as the ejecta 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 the [[ejecta_generic@interpolate]] SUBMODULE).

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 mass density at the point given as argument, in units of $M_\odot/L_\odot^3$.

Arguments

Return Value double precision

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

Returns the pressure at the point given as argument, in units of $M_\odot c^2/L_\odot^3$.

Arguments

Return Value double precision

Pressure at $(x,y,z)$

Returns the spatial metric.

Arguments

Return Value double precision

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

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; return 0 otherwise

Arguments

Return Value logical

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