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We calculate the gravitational wave background produced from density perturbations in an early matter domination era where primordial black holes form.
1904
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I. Hawke and J. M. Stewart, “The dynamics of primordial black hole formation,” Class. Quant. Grav. 19
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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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2012
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2015
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2015
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C. Carbone and S. Matarrese, “A Unified treatment of cosmological perturbations from super-horizon to small scales,” Phys. Rev. D 71
2005
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G. Domènech, S. Pi and M. Sasaki, JCAP 08
2005
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J. Crowder and N. J. Cornish, “Beyond LISA: Exploring future gravitational wave missions,” Phys. Rev. D 72
2005
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2006
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2006
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K. Nakamura, “Second-order gauge invariant cosmological perturbation theory: Einstein equations in terms of gauge invariant variables,” Prog. Theor. Phys. 117
2007
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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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2016
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2016
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2016
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2016
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B. Carr, F. Kuhnel and M. Sandstad, “Primordial Black Holes as Dark Matter,” Phys. Rev. D 94
2016
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2016
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2016
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2017
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S. Sato, S. Kawamura, M. Ando, T. Nakamura, K. Tsubono, A. Araya, I. Funaki, K. Ioka, N. Kanda and S. Moriwaki, et al
2017
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2017
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2017
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2017
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2018
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2018
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2018
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2018
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N. Christensen, “Stochastic Gravitational Wave Backgrounds,” Rept. Prog. Phys. 82
2019
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I. Dalianis, A. Kehagias and G. Tringas, “Primordial black holes from α \alpha -attractors,” JCAP 01
2019
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2019
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2019
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2020
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2020
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T. Nakama, “Stochastic gravitational waves associated with primordial black holes formed during an early matter era,” Phys. Rev. D 101
2020
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