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We investigate some of the experimental, observational and theoreticalconsequences of hypothetical stable black holes in the mass range between theelectro-weak scale and the Planck mass, 2.4$\times 10^{15}$ TeV. For thepurpose of calculations we use Lovelock black holes in odd dimensions. If suchblack holes exist they contribute to dark matter. We show that the passage ofthe black holes through matter and the collision of black holes have a welldefined experimental signature. Depending on their cross section and energythey also accumulate in stars and influence their development.

Do microscopic stable black holes contribute to dark matter?