Overduin, J. M.2017-06-302017-06-3019972017-06-30http://hdl.handle.net/1828/8311Nonstandard cosmological models of two broad classes are examined: those in which there are more than four spacetime dimensions, and those in which there is a variable cosmological “constant” Λ. We test claims that a number of higher-dimensional models give rise to inflation. New constraints are placed on such models, and a number of them are ruled out. We then investigate the potential of variable-Λ theories to address the problem of the initial singularity. We consider a number of different phenomenological representations for this parameter, assessing their implications for the evolution of the cosmological scale factor as well as a range of observational data. In several cases we find nonsingular models which are compatible with observation.enAvailable to the World Wide WebAstronomyCosmologyConstraints (Physics)Observational constraints on higher-dimensional and variable-[lambda] cosmologiesThesis