Gravitational waves from an eccentric population of primordial black holes orbiting Sgr 
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Bondani, Stefano; Bonetti, Matteo; Broggi, Luca; Haardt, Francesco; Sesana, Alberto; Dotti, Massimo

doi:10.1103/physrevd.109.043005

Phys. Rev. D

2024

DOI: 10.1103/physrevd.109.043005

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Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A*

Stefano Bondani,

Matteo Bonetti,

Luca Broggi

et al.

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Primordial Black Hole Messenger of Dark Universe

Khlopov

2024

Symmetry

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Primordial black holes (PBH), if survive to the present time, can be a fraction, or even the dominant form of dark matter of the Universe. If PBH evaporate before the present time, rare forms of dark matter like superweakly interacting or supermassive particles can be produced in the course of their evaporation. Stable remnants of PBH evaporation can also play the role of dark matter candidates. In the context of the modern standard cosmology, based on inflationary models with baryosynthesis and dark matter, which find their physical grounds beyond the Standard models of elementary particles (BSM), primordial black holes acquire the important role of sensitive probes for BSM models and their parameters. It makes PBHs a profound messenger of physics of Dark Universe.

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Primordial Black Hole Messenger of Dark Universe

Khlopov

2024

Symmetry

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Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A*

Cited by 1 publication

References 50 publications

Primordial Black Hole Messenger of Dark Universe

Primordial Black Hole Messenger of Dark Universe

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