2015/07/26 by Renxin Xu, Xu, Renxin
Physics and Astronomy · #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Nuclear Theory (nucl-th) #astro-ph.HE #nucl-th
paper · pdf · doi:10.48550/arxiv.1507.07172
3 pages, 1 figure. Proceeding of "Quarks and Compact Stars 2014 at KIAA (Beijing)"
arxiv created 2015/07/26 · arxiv updated 2015/07/28
The state of cold bulk matter at around nuclear density depends on the fundamental strong interaction between quarks at low-energy scale, so-called non-perturbative quantum chromo-dynamics. Such kind of matter is conjectured to be condensed matter of 3-flavour (u, d and s) quark clusters in this note, being manifested in the form of compact stars, cosmic rays, and even dark matter.