Gravitational wave stochastic background from cosmic (super)strings

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dc.creatorSiemens, Xavier
dc.creatorMandic, Vuk
dc.creatorCreighton, Jolien
dc.date2006-10-30
dc.date2007-02-20
dc.date.accessioned2026-07-07T10:24:04Z
dc.date.available2026-07-07T10:24:04Z
dc.descriptionWe 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.
dc.descriptionReplaced with version accepted for publication in Physical Review Letters. 4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0610920
dc.identifierhttp://arxiv.org/abs/astro-ph/0610920
dc.identifierPhys.Rev.Lett.98:111101,2007
dc.identifierdoi:10.1103/PhysRevLett.98.111101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176056
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational wave stochastic background from cosmic (super)strings
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