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Gravitational-Wave Stochastic Background from Cosmic Strings

2006/10/31 by Xavier Siemens, V. Mandic, Vuk Mandic +2 · 6 citations
Physics and Astronomy · #Astronomy #Astrophysics #Cosmic microwave background #Cosmic string #Cosmology and Gravitation Theories #Einstein Telescope #Gravitational wave #Gravitational-wave observatory #Interferometry #LIGO #Optics #Particle physics theoretical and experimental studies #Physics #Pulsar #Pulsars and Gravitational Waves Research #String (physics) #Theoretical physics #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevlett.98.111101

published as Phys.Rev.Lett.98:111101,2007 · Replaced with version accepted for publication in Physical Review Letters. 4 pages, 2 figures

arxiv created 2007/02/20 · openalex publication_date 2007/03/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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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