I am reading this article on extrinsic curvature embedding diagrams in general relativity: it seems that these are used to visualize curved space. On page 2, it is stated that in the case of the constant Schwarzschild time hypersurface in a Schwarzschild spacetime, the extrinsic curvature embedding is a flat surface. Does that mean that if you take the $t=0$ hypersurface in Schwarzchild spacetime (ie. the spatial part of the Schwarzchild metric) given by
$g_{SC}= \Bigg(1 + \frac{m_0}{2 r} \Bigg) \delta$
that the extrinsic curvature $k_{ij}$ of this hypersurface is just the flat metric $\delta_{ij}$?