Gravitational Wave Background in the Quasi-Steady State Cosmology
  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.
