2019, Vol.22, No.4, pp.311 - 317
New forms of matter such as super-hypernuclei (strange quark matter) and superhypernuclear stars (strange quark stars) as candidates for dark matter are discussed in some detail, based on the so-called "Bodmer–Terazawa–Witten hypothesis" assuming that they are stable absolutely or quasi-stable (decaying only weakly).
Key words: super-hypernuclei, strange quark matter, dark matter
DOI: https://doi.org/10.33581/1561-4085-2019-22-4-311-317
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