Spectrum of cosmic gravitational wave background
| dc.creator | Brustein, Ram | |
| dc.date | 1996-04-25 | |
| dc.date | 1996-06-16 | |
| dc.date.accessioned | 2026-07-07T09:04:20Z | |
| dc.date.available | 2026-07-07T09:04:20Z | |
| dc.description | Models of string cosmology predict a stochastic background of gravitational waves with a spectrum that is strongly tilted towards high frequencies. I give simple approximate expressions for spectral densities of the cosmic background which can be directly compared with sensitivities of gravitational wave detectors. | |
| dc.description | Extrapolation formula and one typo corrected. Latex, 6 pages, 2 eps figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/9604159 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9604159 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/149336 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Spectrum of cosmic gravitational wave background | |
| dc.type | text |