Gravitational Radiation from String Cosmology

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dc.creatorBrustein, R.
dc.creatorGasperini, M.
dc.creatorGiovannini, M.
dc.creatorVeneziano, G.
dc.date1995-10-12
dc.date.accessioned2026-07-07T04:21:32Z
dc.date.available2026-07-07T04:21:32Z
dc.descriptionA spectrum of relic stochastic gravitational radiation, strongly tilted towards high frequencies, and characterized by two basic parameters is shown to emerge in a class of string theory models. We estimate the required sensitivity for detection of the predicted gravitational radiation and show that a region of our parameter space is within reach for some of the plannedgravitational-wave detectors.
dc.description4 pages, uuencoded ps
dc.identifierhttps://arxiv.org/abs/hep-th/9510081
dc.identifierhttp://arxiv.org/abs/hep-th/9510081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54360
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational Radiation from String Cosmology
dc.typetext

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