We discuss the evolution of the bubbles of quark matter which survive from the first-order confinement phase transition till the increase of the internal pressure stops their contraction. We also show that at low temperature and high pressure a quark matter composition u d s is preferred to u d d. We finally describe the different colour superconducting phases which may be formed inside neutron stars, and the topological defects that can be generated, where the stable strangelets might be originated and perhaps already detected at high-altitude observatories.
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机译:我们讨论了夸克泡沫泡沫的演变,从一阶限制相转变中存活,直到内部压力的增加阻止了它们的收缩。我们还表明,在低温和高压下,夸克物质组合物U D S优选为U D D.我们最终描述了可以形成在中子恒星内的不同颜色超导相,以及可以产生的拓扑缺陷,其中稳定的施阵在高空观察者处已经检测到。
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