http://arxiv.org/abs/1505.05494
This paper calculates the expected gravitational wave background (GWB) in the quasi-steady state cosmology (QSSC). The principal sources of gravitational waves in the QSSC are the minicreation events (MCE). With suitable assumptions the GWB can be computed both numerically and with analytical methods. It is argued that the GWB in QSSC differs from that predicted for the standard cosmology and a future technology of detectors will be able to decide between the two predictions. We also derive a formula for the flux density of a typical extragalactic source of gravitational waves.
J. Narlikar, S. Dhurandhar, R. Vishwakarma, et. al.
Thu, 21 May 15
9/59
Comments: Accepted for publication in the MNRAS
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