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Assuming that primordial black holes compose a fraction of dark matter, some of them may accumulate at the center of galaxy and perform a prograde or retrograde orbit against the gravity pointing towards the center exerted by the central massive black hole.
1901
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P. Tisserand et al. (EROS-2), “Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds,” Astron. Astrophys. 469
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2011
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2011
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Pablo A. Rosado, “Gravitational wave background from binary systems,” Phys. Rev. D84
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2013
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2013
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Joseph D. Romano and Neil. J. Cornish, “Detection methods for stochastic gravitational-wave backgrounds: a unified treatment,” Living Reviews in Relativity 20
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2018
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Rory Smith and Eric Thrane, “Optimal search for an astrophysical gravitational-wave background,” Phys. Rev. X 8
2018
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2019
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Sergei V. Ketov and Maxim Yu. Khlopov, “Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales,” Symmetry 11
2019
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