Peak and end point of the relic graviton background in string cosmology

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...

Descripción completa

Detalles Bibliográficos
Autores principales: Brustein, R., Gasperini, M., Veneziano, G.
Lenguaje:eng
Publicado: 1996
Materias:
Particle Physics - Theory
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.55.3882
http://cds.cern.ch/record/301274
_version_ 1780889503947292672
author Brustein, R.
Gasperini, M.
Veneziano, G.
author_facet Brustein, R.
Gasperini, M.
Veneziano, G.
author_sort Brustein, R.
collection CERN
description 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.
id cern-301274
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1996
record_format invenio
spelling cern-3012742023-03-12T05:57:00Zdoi:10.1103/PhysRevD.55.3882http://cds.cern.ch/record/301274engBrustein, R.Gasperini, M.Veneziano, G.Peak and end point of the relic graviton background in string cosmologyParticle Physics - TheoryUsing 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.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.hep-th/9604084CERN-TH-96-37BGU-PH-96-05CERN-TH-96-037BGU-PH-96-05oai:cds.cern.ch:3012741996-04-16
spellingShingle Particle Physics - Theory
Brustein, R.
Gasperini, M.
Veneziano, G.
Peak and end point of the relic graviton background in string cosmology
title Peak and end point of the relic graviton background in string cosmology
title_full Peak and end point of the relic graviton background in string cosmology
title_fullStr Peak and end point of the relic graviton background in string cosmology
title_full_unstemmed Peak and end point of the relic graviton background in string cosmology
title_short Peak and end point of the relic graviton background in string cosmology
title_sort peak and end point of the relic graviton background in string cosmology
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.55.3882
http://cds.cern.ch/record/301274
work_keys_str_mv AT brusteinr peakandendpointoftherelicgravitonbackgroundinstringcosmology
AT gasperinim peakandendpointoftherelicgravitonbackgroundinstringcosmology
AT venezianog peakandendpointoftherelicgravitonbackgroundinstringcosmology

Ejemplares similares