Cosmological application of L0 Riemannian metric and curvature tensor. The flat (k=0) matter-dominated FLRW metric ds² = −dt² + a(t)²(dx²+dy²+dz²) with a(t)=t^{2/3} is the unique cosmological solution of the Einstein equations with a…
Cosmological application of L0 Riemannian metric and curvature tensor. The flat (k=0) matter-dominated FLRW metric ds² = −dt² + a(t)²(dx²+dy²+dz²) with a(t)=t^{2/3} is the unique cosmological solution of the Einstein equations with a…