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arXiv · 1706.04707

Strangeon Stars

Jiguang Lu·Renxin Xu
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Abstract

Stable micro-nucleus is 2-flavored (u and d), whereas stable macro-nucleus could be 3-flavored (u, d and s) if the light flavor symmetry restores there. Nucleons are the constituent of a nucleus, while strangeons are named as the constituent of 3-flavored baryonic matter. Gravity-compressed baryonic object created after core-collapse supernova could be strangeon star if the energy scale (~0.5 GeV) cannot be high enough for quark deconfinement and if there occurs 3-flavor symmetry restoration. Strangeon stars are explained here, including their formation and manifestation/identification. Much work, coupled with effective {micro-model} of strangeon matter, is needed to take advantage of the unique opportunities advanced facilities will provide.

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Jiguang Lu, Renxin Xu. 2017-06-15. Strangeon Stars. https://doi.org/10.7566/jpscp.20.011026

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