This thesis provides generalization to known solutions for the scale factor and cosmic time of Friedmann-Lemaître-Robertson-Walker model universes in terms of elliptic functions. In particular the integration of known expressions for the scale factor is used to find new expressions for cosmic time. Various techniques using both the Weierstrass and Jacobi functions are discussed. Plots of physically significant quantities such as redshift and redshift drift are given. Limiting cases provide context for how various cosmic fluids change the dynamics of the universe on the largest scales.
