2014/02/02 by M. Yu. Khlopov · 2 citations
Physics and Astronomy · #astro-ph.CO #hep-ph
paper · pdf · doi:10.1142/s0217751x14430027
Prepared for a special issue on direct dark matter searches of International Journal of Modern Physics A
arxiv created 2014/02/02 · arxiv updated 2015/06/18
The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new conserved quantum numbers. Dark matter candidates can appear in the new families of quarks and leptons and the existence of new stable charged leptons and quarks is possible, if they are hidden in elusive "dark atoms". Such possibility, strongly restricted by the constraints on anomalous isotopes of light elements, is not excluded in scenarios that predict stable double charged particles. The excessive -2 charged particles are bound in these scenarios with primordial helium in O-helium "atoms", maintaining specific nuclear-interacting form of the dark matter, which may provide an interesting solution for the puzzles of the direct dark matter searches.