1996/04/16 by Ram Brustein, R. Brustein, M. Gasperini +1 · 78 citations
Mathematics · Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Geometry #Gravitation #Gravitational wave #Graviton #Mathematics #Physics #Point (geometry) #Pulsars and Gravitational Waves Research #Quantum gravity #Quantum mechanics #Range (aeronautics) #Sensitivity (control systems) #Statistical physics #String (physics) #String cosmology #Theoretical physics #astro-ph #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.55.3882
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 55(6), 3882-3885 (American Physical Society) · 11 pages, LATEX, one figure included using eps. A complete collection of papers and references on the pre-big-bang scenario in string cosmology is available at http://www.to.infn.it/teorici/gasperini/
arxiv created 1996/04/16 · openalex publication_date 1997/03/15 · arxiv updated 2011/09/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Using general arguments we determine the allowed region for the end point frequency and the peak energy density of the stochastic background of gravity waves expected in string cosmology. We provide an accurate estimate of the minimal experimental sensitivity required to detect a signal in the Hz to GHz range.