Method

NumCosmoWLSurfaceMassDensitymagnification

Declaration [src]

gdouble
nc_wl_surface_mass_density_magnification (
  NcWLSurfaceMassDensity* smd,
  NcHaloDensityProfile* dp,
  NcHICosmo* cosmo,
  const gdouble R,
  const gdouble zs,
  const gdouble zl,
  const gdouble zc
)

Description [src]

Computes the reduced shear: $$ \mu(R) = \frac{1}{(1 - \kappa(R))^2 - \vert\gamma^2(R) \vert},$$ where $\gamma(R)$ is the shear [nc_wl_surface_mass_density_shear()] and $\kappa(R)$ is the convergence [nc_wl_surface_mass_density_convergence()].

Parameters

dp

Type: NcHaloDensityProfile

A NcHaloDensityProfile.

The data is owned by the caller of the method.
cosmo

Type: NcHICosmo

A NcHICosmo.

The data is owned by the caller of the method.
R

Type: const gdouble

Projected radius with respect to the center of the lens / halo.

zs

Type: const gdouble

Source redshift $z_\mathrm{source}$.

zl

Type: const gdouble

Lens redshift $z_\mathrm{lens}$.

zc

Type: const gdouble

Cluster redshift $z_\mathrm{cluster}$.

Return value

Type: gdouble

$\mu(R)$.