arXiv · hep-th/9502130
EVOLUTION OF A STRING NETWORK IN BACKGROUNDS WITH ROLLING HORIZONS
Abstract
We discuss the temporal variation of the equation of state of a classical string network, evolving in a background in which the Hubble radius 1/H shrinks to a minimum and then re-expands to infinity. We also present a method to look for self-consistent non-vacuum string backgrounds, correponding to the simultaneous solution of the gravi-dilaton backgrounds equations and of the string equations of motion.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. Gasperini, M. Giovannini, K. A. Meissner, G. Veneziano. 1995-02-22. EVOLUTION OF A STRING NETWORK IN BACKGROUNDS WITH ROLLING HORIZONS. https://arxiv.org/abs/hep-th/9502130
Cite the original work for its findings. Save a collection to share your selection of sources.