Investigation of compact stars with heavy baryons and quarks: second period

本项目旨在继续研究重重子（如超子和三角洲共振）和定义夸克物质的状态稠密物质方程。本文将研究在有限温度条件下，中子星合并和超新星爆炸中出现的热致密星的状态方程。涉及δ共振的弱相互作用速率将被导出并用于中微子与物质相互作用和中子星长期冷却的研究。

This project is aimed at contrinuing the study of the equation of state dense matter featuring heavy baryons, such as hyperons andDelta-resonances, as well as deconfined quark matter. The equation of state will be studied under the conditions of finite temperaturerelevant for hot compact stars, that emerge in binary-neutron-star mergers and supernova explosions. The weak interaction rates involving Delta-resonances will be derived and used for the studies of neutrino interactions with matter and long-term cooling of neutron stars.