Nuclear clusters or voids in the inner crust of neutron stars were predicted to have various shapes collectively nicknamed nuclear pasta. The recent review in Ref. [1] by López, Dorso and Frank summarized their systematic investigations into properties especially the morphological and thermodynamical phase transitions of the nuclear pasta within a Classical Molecular Dynamics model, providing further stimuli to find more observational evidences of the predicted nuclear pasta in neutron stars.

中文翻译：

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用经典的分子动力学模拟品尝核面食

预计中子星内壳中的核簇或空隙具有各种形状，统称为“核面食”。参考文献中的最新评论。[1]由López，Dorso和Frank总结了他们对经典分子动力学模型中核面食的特性，特别是形态和热力学相变的系统研究，为进一步寻找发现中子星中预测的核面食的证据提供了进一步的刺激。