Gravitational wave stochastic background from cosmic (super)strings
Loading...
Date
Journal Title
Journal ISSN
Volume Title
Publisher
Abstract
Description
We consider the stochastic background of gravitational waves produced by a network of cosmic strings and assess their accessibility to current and planned gravitational wave detectors, as well as to big bang nucleosynthesis (BBN), cosmic microwave background (CMB), and pulsar timing constraints. We find that current data from interferometric gravitational wave detectors, such as LIGO, are sensitive to areas of parameter space of cosmic string models complementary to those accessible to pulsar, BBN, and CMB bounds. Future more sensitive LIGO runs and interferometers such as Advanced LIGO and LISA will be able to explore substantial parts of the parameter space.
Replaced with version accepted for publication in Physical Review Letters. 4 pages, 2 figures
Replaced with version accepted for publication in Physical Review Letters. 4 pages, 2 figures