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The gravitational potential of initially Poisson distributed primordial black holes (PBH) can induce a stochastic gravitational-wave background (SGWB) at second order in cosmological perturbation theory.
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J. C. Niemeyer and K. Jedamzik, Near-critical gravitational collapse and the initial mass function of primordial black holes , Phys. Rev. Lett. 80
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J. C. Niemeyer and K. Jedamzik, Dynamics of primordial black hole formation , Phys. Rev. D 59
1999
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M. Kawasaki, K. Kohri and N. Sugiyama, MeV scale reheating temperature and thermalization of neutrino background , Phys. Rev. D 62
2000
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D. Wands, K. A. Malik, D. H. Lyth and A. R. Liddle, A New approach to the evolution of cosmological perturbations on large scales , Phys.Rev. D62
2000
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M. Maggiore, Gravitational wave experiments and early universe cosmology , Phys. Rept. 331
2000
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R. Bean and J. Magueijo, Could supermassive black holes be quintessential primordial black holes? , Phys. Rev. D 66
2002
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2002
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N. Afshordi, P. McDonald and D. Spergel, Primordial black holes as dark matter: The Power spectrum and evaporation of early structures , Astrophys. J. Lett. 594
2003
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2013
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T. Nakama and T. Suyama, Primordial black holes as a novel probe of primordial gravitational waves , Physical Review D 92
2015
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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
2017
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V. Desjacques and A. Riotto, Spatial clustering of primordial black holes , Phys. Rev. D 98
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G. Domènech, Scalar Induced Gravitational Waves Review , Universe 7
2021
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2022
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