  The exact renormalization group flow equations for gravity lead to quantum
corrections of Newton's constant and cosmological constant. Using this we
investigate the Bianchi-I cosmological model at late times. In particular, we
obtain the scale factors in different directions, and observe that they
eventually evolve into Friedmann-Lema\^itre-Robertson-Walker (FLRW) universe
for radiation. However, for stiff matter the universe shows a Kasner like
behaviour. The presentation is based on our work published in
\cite{Mandal:2019xlg}.
