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The gravitational potential of a gas of initially randomly distributed primordial black holes (PBH) can induce a stochastic gravitational-wave (GW) background through second-order gravitational effects.
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S. Nojiri and S. D. Odintsov, Modified f(R) gravity consistent with realistic cosmology: From matter dominated epoch to dark energy universe , Phys. Rev. D 74
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W. Hu and I. Sawicki, Parametrized post-friedmann framework for modified gravity , Phys. Rev. D 76
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K. N. Ananda, C. Clarkson and D. Wands, The Cosmological gravitational wave background from primordial density perturbations , Phys. Rev. D75
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2015
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G. Janssen et al., Gravitational wave astronomy with the SKA , PoS AASKA14
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J.-c. Hwang, D. Jeong and H. Noh, Gauge dependence of gravitational waves generated from scalar perturbations , The Astrophysical Journal 842
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W. C. Rubén Arjona and S. Nesseris, Unraveling the effective fluid approach for f(R) models in the subhorizon approximation , Phys. Rev. D 99, 043516 99
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G. Domènech, Scalar Induced Gravitational Waves Review , Universe 7
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E. N. Saridakis, Do we need soft cosmology? , Phys. Lett. B 822
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