Affiliation:
1. Department of Mathematics and Physics “Ennio de Giorgi”, University of Salento, Lecce, Italy
Abstract
We discuss the hypothesis that the constituents of dark matter in the galactic halo are primordial intermediate-mass black holes (PIMBHs). The status of axions and weakly interacting massive particles (WIMPs) is discussed, as are the methods for detecting PIMBHs with emphasis on microlensing. The role of the angular momentum [Formula: see text] of the PIMBHs in their escaping previous detection is considered.
Publisher
World Scientific Pub Co Pte Lt
Subject
General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics
Cited by
1 articles.
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