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Gravitational-Wave Stochastic Background from Cosmic Strings

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Siemens, Xavier, Mandic, Vuk, Creighton, Jolien·2007·Physical Review Letters

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.

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Metadata

Authors
Siemens, X., Mandic, V., & Creighton, J.
Venue
Physical Review Letters
Published
2007-03-13
Volume
98
Issue
11
Pages
111101-111101
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2076655426
Cited by
311
References
0
FWCI
11.27
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Gravitational-Wave Stochastic Background from Cosmic Strings. https://app.cochat.ai/papers/10.1103/physrevlett.98.111101
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Siemens, X., Mandic, V., & Creighton, J. (2007). Gravitational-Wave Stochastic Background from Cosmic Strings. Physical Review Letters. https://doi.org/10.1103/physrevlett.98.111101

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