Abstract

We consider a model of OOHe atomic dark matter formed by Coulomb binding of the hypothetical stable double-charged massive O−−O^{--} particles with nuclei of primordial helium. Such a dark matter can be captured by ordinary matter forming superheavy nuclei. We propose a possibility of self-bound by nuclear and electromagnetic interaction OO-nuclearites as well as more massive gravitating ones and discuss effect of accumulation of OOHe atoms in stars and their effect in stellar evolution.

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