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Primordial black holes and secondary gravitational waves can be used to probe the small scale physics at very early time.
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R. J. Nemiroff, G. F. Marani, J. P. Norris and J. T. Bonnell, Limits on the cosmological abundance of supermassive compact objects from a millilensing search in gamma-ray burst data , Phys. Rev. Lett. 86
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S. Mollerach, D. Harari and S. Matarrese, CMB polarization from secondary vector and tensor modes , Phys. Rev. D 69
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M. Yu. Khlopov, S. G. Rubin and A. S. Sakharov, Primordial structure of massive black hole clusters , Astropart. Phys. 23
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K. N. Ananda, C. Clarkson and D. Wands, The Cosmological gravitational wave background from primordial density perturbations , Phys. Rev. D 75
2007
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D. Baumann, P. J. Steinhardt, K. Takahashi and K. Ichiki, Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations , Phys. Rev. D 76
2007
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H. Motohashi and W. Hu, Primordial Black Holes and Slow-Roll Violation , Phys. Rev. D 96
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2010
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M. Drees and E. Erfani, Running-Mass Inflation Model and Primordial Black Holes , JCAP 1104
2011
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2017
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W.-R. Hu and Y.-L. Wu, The Taiji Program in Space for gravitational wave physics and the nature of gravity , Natl. Sci. Rev. 4
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Z. Yi and Y. Gong, On the constant-roll inflation , JCAP 1803
2018
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