Speaker
Min Ju
(中国石油大学（华东）)
Description
Neutron stars are considered as the ideal natural laboratories to study the physics of dense matter, where the matter covers a huge range of densities. The baryon number density in the core of the neutron star can reach 5-10 $n_0$ ($n_0 \sim 0.16\ \rm{fm}^{-3}$), so the hadron-quark deconfinement phase transition is likely to occur. Traditionally, the hadron-quark phase transition in neutron stars has been assumed to be first-order. This naturally suggests that during the transition, the system exists in a mixed phase state. In recent years, we have systematically investigated the potential formation of a structured hadron-quark mixed phase within neutron star interiors. In this report, I will present the results of our calculations.
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Author
Min Ju
(中国石油大学（华东）)