Relic gravitational waves from string cosmology

R. Brustein; M. Gasperini; M. Giovannini; G. Veneziano

doi:10.1016/0370-2693(95)01128-D

Relic gravitational waves from string cosmology

R. Brustein
, M. Gasperini
, M. Giovannini
, G. Veneziano

Department of Physics

Research output: Contribution to journal › Article › peer-review

210 Scopus citations

Abstract

A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational waves, strongly tilted towards high frequencies, and characterized by two basic parameters of the cosmological model. 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 planned gravitational-wave detectors.

Original language	English
Pages (from-to)	45-51
Number of pages	7
Journal	Physics Letters B
Volume	361
Issue number	1-4
DOIs	https://doi.org/10.1016/0370-2693(95)01128-D
State	Published - 2 Nov 1995

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0370-2693(95)01128-D

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@article{f9d9e90c128f4126bd1904f5d28e5f5e,

title = "Relic gravitational waves from string cosmology",

abstract = "A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational waves, strongly tilted towards high frequencies, and characterized by two basic parameters of the cosmological model. 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 planned gravitational-wave detectors.",

author = "R. Brustein and M. Gasperini and M. Giovannini and G. Veneziano",

year = "1995",

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doi = "10.1016/0370-2693(95)01128-D",

language = "English",

volume = "361",

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journal = "Physics Letters B",

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TY - JOUR

T1 - Relic gravitational waves from string cosmology

AU - Brustein, R.

AU - Gasperini, M.

AU - Giovannini, M.

AU - Veneziano, G.

PY - 1995/11/2

Y1 - 1995/11/2

N2 - A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational waves, strongly tilted towards high frequencies, and characterized by two basic parameters of the cosmological model. 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 planned gravitational-wave detectors.

AB - A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational waves, strongly tilted towards high frequencies, and characterized by two basic parameters of the cosmological model. 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 planned gravitational-wave detectors.

UR - https://www.scopus.com/pages/publications/13844323292

U2 - 10.1016/0370-2693(95)01128-D

DO - 10.1016/0370-2693(95)01128-D

M3 - Article

AN - SCOPUS:13844323292

SN - 0370-2693

VL - 361

SP - 45

EP - 51

JO - Physics Letters B

JF - Physics Letters B

IS - 1-4

ER -

Relic gravitational waves from string cosmology

Abstract

ASJC Scopus subject areas

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