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Oznake: primordial black holes;QCD phase transitionž;threshold;mass distribution;abundance;
Primordial black hole (PBH) formation during cosmic phase transitions and annihilation periods, such as the QCD transition or the e+e- annihilation, is thought to be particularly efficient due to a softening of the equation of state. We present a detailed numerical study of PBH formation during the ...
Leto: 2024 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
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