Abstract
Observational upper limits on the abundance of primordial black holes can be considered as a method to get non-trivial upper limits on the spectrum of initial metric perturbations and physical conditions in the very early Universe.
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© 1989 Springer-Verlag
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Polnarev, A.G. (1989). Primordial black holes and their cosmological consequences. In: Flin, P., Duerbeck, H.W. (eds) Morphological Cosmology. Lecture Notes in Physics, vol 332. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-51223-3_137
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DOI: https://doi.org/10.1007/3-540-51223-3_137
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