What were the relative energy densities in the early Universe? (below, DE means dark energy)
(a) They remain roughly equal: �rad ∼ �mat ∼ �DE
(b) �DE > �mat > �rad
(c) �rad > �mat > �DE
(d) �mat > �rad > �DE
(a) They remain roughly equal: �rad ∼ �mat ∼ �DE
(b) �DE > �mat > �rad
(c) �rad > �mat > �DE
(d) �mat > �rad > �DE