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arXiv physics/0209024physics.flu-dynastro-phcond-mat
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多流体动力学的变分描述:不带电流体

Variational description of multi-fluid hydrodynamics: Uncharged fluids

Reinhard Prix

摘要:

本文从无约束变分原理出发,给出了牛顿多流体动力学的一种形式。这种方法提供了一种自然的方式来获得广泛的流体动力学系统的一般运动方程包含任意数量的相互作用的流体和超流体。除了空间变化,我们在变分原理中使用"时移“,这使我们能够描述具有熵产生的耗散过程,例如化学反应、摩擦或外部非保守力的影响。由此产生的框架纳入了最初讨论的情况下,由Andreev和Bashkin的两个超流体的混合物的夹带效应的推广。除了能量守恒和动量守恒外,我们还导出了涡度和螺旋度的广义守恒律,以及Ertel定理在单一理想流体中的特例。我们明确地讨论了这个框架的应用,热传导流体,超流体和超流体中子星的问题。控制导热流体的方程被发现比标准描述更一般,因为在这种情况下夹带的影响通常似乎被忽略了。在超流He 4的情况下,我们恢复的Landau-Khalatnikov方程的双流体模型通过翻译的“正统”框架的超流性,这是基于一个相当尴尬的选择变量。我们的超流中子星物质的双流体模型允许通过相互摩擦进行耗散,也允许通过中子流体和质子-电子流体之间的β反应进行“输血”。

英文摘要:

We present a formalism for Newtonian multi-fluid hydrodynamics derived from an unconstrained variational principle. This approach provides a natural way of obtaining the general equations of motion for a wide range of hydrodynamic systems containing an arbitrary number of interacting fluids and superfluids. In addition to spatial variations we use ``time shifts'' in the variational principle, which allows us to describe dissipative processes with entropy creation, such as chemical reactions, friction or the effects of external non-conservative forces. The resulting framework incorporates the generalization of the entrainment effect originally discussed in the case of the mixture of two superfluids by Andreev and Bashkin. In addition to the conservation of energy and momentum, we derive the generalized conservation laws of vorticity and helicity, and the special case of Ertel's theorem for the single perfect fluid. We explicitly discuss the application of this framework to thermally conducting fluids, superfluids, and superfluid neutron star matter. The equations governing thermally conducting fluids are found to be more general than the standard description, as the effect of entrainment usually seems to be overlooked in this context. In the case of superfluid He4 we recover the Landau--Khalatnikov equations of the two-fluid model via a translation to the ``orthodox'' framework of superfluidity, which is based on a rather awkward choice of variables. Our two-fluid model for superfluid neutron star matter allows for dissipation via mutual friction and also ``transfusion'' via beta-reactions between the neutron fluid and the proton-electron fluid.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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