Cosmological Euler equation in synchronous gauge
= Cosmological Euler equation in synchronous gauge
{c}
For scalar perturbations of a generic fluid in cosmic time, momentum conservation in <synchronous gauge in cosmology> gives
$$
\delta P+\nabla^2\pi^S
+\partial_t[(\bar\rho+\bar P)\delta u]
+3H(\bar\rho+\bar P)\delta u=0.
$$