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Hyperonová hvězda je hypotetický stav, ve kterém se nachází jádro hvězdy po supernově, když jeho hmotnost byla vyšší než 2× hmotnost Slunce a přitom nižší než Tolmanova–Oppenheimerova–Volkoffova mez (občas nazývaná Landauova-Opppenheimerova-Volkoffova mez), tedy 3–5 Sluncí. Hustoty hyperonové hvězdy by se měly pohybovat mezi 1015–1017 kg.m³, což je horní…
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hvězdy hyperonové jsou suprakapaliny neutronové neutronových hvězd plazma složeny jako hyperony složky spolu supernově slunce kvarky kvarkovou hyperonů elektron tetrakvark
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