Some properties of convection in hybrid stars
Some properties of convection in hybrid stars
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混合星中对流的一些性质
DOI：
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发表时间：
2015
期刊：
影响因子：
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通讯作者：
T. L. Razinkova
中科院分区：
文献类型：
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作者：
A. Yudin;M. Hempel;D. Nadyozhin;T. L. Razinkova
结果表明，混合星中两相共存区域物质的异常热力学性质导致了对流开始的标准条件的改变。具体地说，对流输送的热通量可能指向恒星中心。我们讨论了导致这种“逆对流”效应的有利条件，以及它对混合星热演化的可能影响。
It is shown that the unusual thermodynamic properties of matter within the region of two-phase coexistence in hybrid stars result in a change of the standard condition for beginning of convection. In particular, the thermal flux transported by convection may be directed towards the stellar centre. We discuss favourable circumstances leading to such an effect of ‘inverse convection’ and its possible influence on the thermal evolution of hybrid stars.