2016, Vol.19, No.2, pp.147-152
New forms of matter such as super-hypernuclei(strange quark matter) and superhypernuclear stars(strange quark stars) are discussed in some detail, based on the so-called “Bodmer–Terazawa–Witten hypothesis” assuming that they are stable or quasi-stable.
Key words: strange quark matter, super-hypernuclear stars
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