Production and detection of cosmic gravitational wave background in string cosmology

DOI10.1016/S0960-0779(98)00196-9zbMATH Open1009.83016arXivgr-qc/9810063MaRDI QIDQ1610007

R. Brustein

Publication date: 18 August 2002

Published in: Chaos, Solitons and Fractals (Search for Journal in Brave)

Abstract: String cosmology models predict a cosmic background of gravitational waves produced during a period of dilaton-driven inflation. I describe the background, present astrophysical and cosmological bounds on it, and discuss in some detail how it may be possible to detect it with large operating and planned gravitational wave detectors. The possible use of smaller detectors is outlined.

Full work available at URL: https://arxiv.org/abs/gr-qc/9810063

zbMATH Keywords

cosmic gravitational wave backgroundmodels of string cosmology

Mathematics Subject Classification ID

String and superstring theories in gravitational theory (83E30) Gravitational waves (83C35)

Cites Work

• The early universe. With a foreword by David Pines

Related Items (2)

String interactions in gravitational wave backgrounds ⋮ Gravitational waveforms from the evaporating ACO cosmic string loop

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