Massive Hybrid Stars with Strangeness
arXiv:1402.4677 · doi:10.1142/9789814618229_0037
Abstract
How massive the hybrid stars could be is discussed by a "3-window model" proposed from a new strategy to construct the equation of state with hadron-quark transition. It is found that hybrid stars have a strong potentiality to generate a large mass compatible with two-solar-mass neutron star observations.
4 pages,1 figure