Relic Gravitational Waves from String Cosmology
classification
✦ hep-th
astro-phgr-qc
keywords
gravitationalrelicwavesbackgroundsbasiccharacterizedclasscosmological
read the original abstract
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational waves, strongly tilted towards high frequencies, and characterized by two basic parameters of the cosmological model. We estimate the required sensitivity for detection of the predicted gravitational radiation and show that a region of our parameter space is within reach for some of the planned gravitational-wave detectors.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Science Case for the Einstein Telescope
The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.