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• W2066371027 abstract "Abstract Primordial black holes (PBH) may have formed from the collapse of cosmic string loops. The spectral shape of the PBH mass spectrum can be determined by the scaling argument for string networks. Limits on the spectral amplitude derived from extragalactic γ-ray and galactic γ-ray and cosmic ray flux observations as well as constraints from the possible formation of stable black holes remnants are reanalyzed. The new constraints are remarkably close to those derived from the normalization of the cosmic string model to the cosmic microwave background anisotropies." @default.
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• W2066371027 date "1998-12-01" @default.
• W2066371027 modified "2023-09-27" @default.
• W2066371027 title "Astrophysical constraints on primordial black hole formation from collapsing cosmic strings" @default.
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• W2066371027 doi "https://doi.org/10.1016/s0370-1573(98)00070-2" @default.
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