超新星核中的夸克相变及夸克质量效应

Quark phase transition in supernova and the effect of quark mass on the process

分别基于组夸克质量模型和流夸克质量模型,讨论了超新星核心区两味夸克物质到更稳定的三味夸克物质的相变过程.结果表明,两种质量模型下相变的特征时标都短于10-8s,且质量越小的流夸克质量模型的相变速率越快;组分夸克质量模型下所得到的超新星核区的s夸克丰度,中微子丰度及中微子总能量(除温度)相比前人的结果有轻微的增加,而流夸克质量模型下所得到的这些参量的增加更为明显,采用流夸克质量模型更有利于超新星的中微子延迟爆发机理的成功.

Based on constituent quark mass and current quark mass model, the phase transition of two-flavor quark matter to more stable three-flavor quark matter in the core of supernova is studied. It is shown that the timescale of the process is shorter than 10^- 8 seconds for both cases, and the smaller the quark mass （current quark mass）, the quicker the process; and the equilibrium parameters, except the temperature, such as s-quark abundance, neutrino abundance and total neutrino energy in supernova core, have a slight increase compared to the former result after the conversion according to constituent quark mass model. But the values of those parameters （including temperature） increase significantly based on current quark mass model. The current quark mass will be more favorable for the success of the delayed neutrino-heating mechanism for the explosion.