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arXiv 0912.0129nucl-th
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$β$稳定核物质的剪切粘度

Shear viscosity of $β$-stable nuclear matter

Omar Benhar, Arianna Carbone

摘要:

粘性在决定旋转中子星的稳定性方面起着至关重要的作用。我们报告的结果的剪切粘度的计算$β$ ~-~稳定的物质,进行了有效的相互作用的基础上,一个国家的最先进的核子核子势和形式主义的相关基函数。在我们的方法的状态方程,确定质子分数,和核子-核子散射概率一致地从相同的动力学模型。结果表明,虽然中子的贡献总是占主导地位的粘度,核饱和密度以上的电子的贡献变得明显。

英文摘要:

Viscosity plays a critical role in determining the stability of rotating neutron stars. We report the results of a calculation of the shear viscosity of $β$~-~stable matter, carried out using an effective interaction based on a state-of-the-art nucleon-nucleon potential and the formalism of correlated basis functions. Within our approach the equation of state, determining the proton fraction, and the nucleon-nucleon scattering probability are consistently obtained from the same dynamical model. The results show that, while the neutron contribution to the viscosity is always dominant, above nuclear saturation density the electron contribution becomes appreciable.

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