arXiv · gr-qc/9810063
Production and Detection of Cosmic Gravitational Wave Background in String Cosmology
Abstract
String cosmology models predict a cosmic background of gravitational waves produced during a period of dilaton-driven inflation. I describe the background, present astrophysical and cosmological bounds on it, and discuss in some detail how it may be possible to detect it with large operating and planned gravitational wave detectors. The possible use of smaller detectors is outlined.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Ram Brustein. 1998-10-20. Production and Detection of Cosmic Gravitational Wave Background in String Cosmology. https://doi.org/10.1016/s0960-0779(98)00196-9
Cite the original work for its findings. Save a collection to share your selection of sources.