A chiral hadronic model is extended to investigate the influences of trapped neutrinos on the equation of state of dense matter and structure of protoneutron stars.
用手征强子模型研究在中微子束缚情况下对致密物质状态及其对前中子星结构的影响。
A chiral hadronic model is extended to investigate the influences of trapped neutrinos on the equation of state of dense matter and structure of protoneutron stars.
用手征强子模型研究在中微子束缚情况下对致密物质状态及其对前中子星结构的影响。
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