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On the Present Time Approximate Values of the Characteristic Parameters of the Primordial Gravitational Waves

Published online by Cambridge University Press:  26 May 2016

M. Melek
M. Melek*
Affiliation:
Astronomy Department, Faculty of Science, Cairo University, Orman, Giza, Egypt; melek@frcu.eun.eg

Abstract

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An approach is used to find out the present time approximate values of the characteristic amplitudes, the spectral densities, the intensties and the frequencies of the Primordial Gravitational Waves (PmGW), in the spatially perturbed Friedman - Robertson - Walker (FRW) adiabatically expanding Universe. The temporal variation of the magnitude of the time gradient of the characteristic amplitudes of the PmGW is calculated in spatial perturbed FRW Universe. The obtained results via this non-conventional approach may be of interest to shed some light on the possibilities of searching for the PmGW at definite frequency bands by the existing and the future networks of detectors.

Type
Part 10 Non-Photon Astrophysics and the Future
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 376 - 381
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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