Gravitational-wave stochastic background from cosmic strings

Xavier Siemens, Vuk Mandic, Jolien Creighton

Research output: Contribution to journalArticlepeer-review

162 Scopus citations

Abstract

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 Laser Interferometer Gravitational Wave Observatory (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 Laser Interferometer Space Antenna (LISA) will be able to explore substantial parts of the parameter space.

Original languageEnglish (US)
Article number111101
JournalPhysical review letters
Volume98
Issue number11
DOIs
StatePublished - Mar 13 2007

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