论文标题
散装强的问题：三位一体
Bulk Strong Matter: the Trinity
论文作者
论文摘要
我们的世界很棒，因为尽管未知的暗物质和深色能量占据了宇宙的占主导地位，但它正常但可忽略不计的小型男性元素（即原子）。稳定的原子核可以简单地称为``强质''，因为它的性质由基本的强相互作用主导。还有其他形式的有力物质吗？尽管核是由2-泡沫（即价夸克的上下味道）组成的核子，但猜测可以将大量强的强度（带有额外的奇怪夸克）超过临界值超过临界值，$ a _ _ _ _ {\ rm c} $ noveral of Stranch or Strange of trace of trace（因此，否认了（因此），否则（同样）又有奇怪的是（因此，否定了（同样），这是因为否定的（因此，否定了）。通过结合``奇怪的核子''来创造）。散装强的物质可以以紧凑的恒星，宇宙射线甚至暗物质的形式表现出来。这三位一体将在这篇简短的综述中进行解释，该评论可能会对当今的物理学产生巨大影响，尤其是在发现引力波之后的多理性天文学时代。
Our world is wonderful because of the normal but negligibly small baryonic part (i.e., atoms) although unknown dark matter and dark energy dominate the Universe. A stable atomic nucleus could be simply termed as ``strong matter'' since its nature is dominated by the fundamental strong interaction. Is there any other form of strong matter? Although nuclei are composed of 2-flavoured (i.e., up and down flavours of valence quarks) nucleons, it is conjectured that bulk strong matter could be 3-flavoured (with additional strange quarks) if the baryon number exceeds the critical value, $A_{\rm c}$, in which case quarks could be either free (so-called strange quark matter) or localized (in strangeons, coined by combining ``strange nucleon''). Bulk strong matter could be manifested in the form of compact stars, cosmic rays, and even dark matter. This trinity will be explained in this brief review, that may impact dramatically on today's physics, particularly in the era of multi-messenger astronomy after the discovery of gravitational wave.
