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Quantum chromodynamics phase transition in the early Universe and quark nuggets

机译:早期宇宙和夸克块中的量子色动力学相变

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A first-order quark hadron phase transition in the early Universe may lead to the formation of quark nuggets. The baryon number distribution of these quark nuggets have been calculated and it has been found that there are sizeable number of quark nuggets in the stable sector. The nuggets can clump and form bigger objects in the mass range of 0.0003M⊙ to 0.12M⊙. It has been discussed that these bigger objects can be possible candidates for cold dark matter. Keywords Quark nuggets - dark matter - massive astrophysical compact halo objects PACS Nos 98.80.Cq - 12.38.Mh - 95.35.+d
机译:宇宙早期的一阶夸克强子相变可能导致夸克块的形成。计算了这些夸克块的重​​子数分布,发现在稳定区域中存在大量的夸克块。熔核会结块并形成质量范围为0.0003M⊙至0.12M⊙的较大物体。已经讨论过这些较大的物体可能是冷暗物质的候选者。关键词夸克核-暗物质-巨大的天体物理紧凑光晕物体PACS Nos 98.80.Cq-12.38.Mh-95.35。+ d

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