arXiv · hep-th/9801008
String Cosmology: An Update
Abstract
A string cosmology scenario ("pre-big-bang") postulates that the evolution of the Universe starts from a state of very small curvature and coupling, undergoes a long phase of dilaton-driven kinetic inflation and at some later time joins smoothly standard radiation dominated cosmological evolution, thus giving rise to a singularity free inflationary cosmology. I report on recent progress in understanding some outstanding issues such as initial conditions, graceful exit transition and generation of inhomogeneity perturbations.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Ram Brustein. 1998-01-04. String Cosmology: An Update. https://doi.org/10.1142/9789814447263_0077
Cite the original work for its findings. Save a collection to share your selection of sources.