Expanding flat slicing of de Sitter spacetime
= Expanding flat slicing of de Sitter spacetime
{c}
The expanding flat slicing has metric
$$
ds^2=-dt^2+e^{2Ht}d\mathbf x^2,
\qquad H>0.
$$
It covers one half of global <de Sitter spacetime> and has a past coordinate boundary at $t\to-\infty$.