用Brueckner-Hartree-Fock方法研究质子中子星和有限温度K介子凝聚
Protoneutron stars in the Brueckner-Hartree-Fock approach and finite-temperature kaon condensation
摘要：
本文采用包含三体力的Brueckner-Hartree-Fock方法中的核物质状态方程，结合有限温度下K介子凝聚的标准手征模型，研究了热中微子俘获的β稳定恒星物质的性质.然后在这个框架内研究了（原）中子星的性质。
英文摘要：
We study the properties of hot neutrino-trapped beta-stable stellar matter using an equation of state of nuclear matter within the Brueckner-Hartree-Fock approach including three-body forces, combined with a standard chiral model for kaon condensation at finite temperature. The properties of (proto)neutron stars are then investigated within this framework.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
