Abstract
Nematodynamics is the orientation dynamics of flowless liquid-crystals. We show how Euler-Poincaré reduction produces a unifying framework for various theories, including Ericksen-Leslie, Luhiller-Rey, and Eringen’s micropolar theory. In particular, we show that these theories are all compatible with each other and some of them allow for more general configurations involving a non vanishing disclination density. All results are also extended to flowing liquid crystals.
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Acknowledgements
Stimulating conversations with David Chillingworth, Giovanni De Matteis, and Giuseppe Gaeta are greatly acknowledged. Also, the authors wish to warmly thank the referees for their valuable comments and keen remarks that helped improving this paper.
TSR was partially supported by Swiss NSF grant 200020-126630 and by the government grant of the Russian Federation for support of research projects implemented by leading scientists, Lomonosov Moscow State University under the agreement No. 11.G34.31.0054.
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Appendix: The Free Energy
Appendix: The Free Energy
We reproduce here the computation in [12] that shows how all terms in the Frank energy
![](http://media.springernature.com/full/springer-static/image/art%3A10.1007%2Fs10440-012-9719-x/MediaObjects/10440_2012_9719_Equcb_HTML.gif)
can be rewritten in terms of the variables j=J(I−n⊗n) and γ, the latter being introduced through the invariant relation ∇n=n×γ. Thus, the explicit expression for the micropolar free energy Ψ(j,γ) of nematic media given in (4.4) will be written after computing the micropolar expression for each term in the Frank energy. Further details are given in [12].
Twist
Using n⊗n=I−j/J, we have
where γ(n)=γ ia n a , with a being the \(\mathfrak{so}(3)\simeq\Bbb{R}^{3}\)-index, and γ S denotes the skew part of γ, i.e., γ S=(γ−γ T)/2, where we see γ as a 3×3 matrix with components γ ia .
Splay
We introduce the vector \({\vec{{\boldsymbol {\gamma }}} }_{b}=\epsilon_{abc}{\boldsymbol {\gamma }}_{ac}\), defined by the condition \(\vec{\boldsymbol{\gamma }} \cdot\mathbf{u}=\operatorname{Tr}(\mathbf{u}\times\boldsymbol{\gamma})\), for all u∈ℝ3, where u×γ is the matrix with components (u×γ) ia =(u×γ i ) a . We compute
![](http://media.springernature.com/full/springer-static/image/art%3A10.1007%2Fs10440-012-9719-x/MediaObjects/10440_2012_9719_Equcd_HTML.gif)
where γ A denotes the skew part of γ, i.e., γ A=(γ−γ T)/2 and where we used the equality \(\widehat{\vec{\boldsymbol{\gamma}}} =-2\boldsymbol{\gamma}^{A}\). The latter can be shown by noting that we have the equalities \(\operatorname{Tr}(\widehat{\vec{\boldsymbol{\gamma}}}\hat {\mathbf{u}})=-2\vec{\boldsymbol{\gamma}}\cdot\mathbf{u}=-2\operatorname{Tr}(\boldsymbol{\gamma}\widehat{\mathbf{u}})\) for all u∈ℝ3.
Bend
For all u∈ℝ3, we have
![](http://media.springernature.com/full/springer-static/image/art%3A10.1007%2Fs10440-012-9719-x/MediaObjects/10440_2012_9719_Equce_HTML.gif)
so we get
and therefore
Summing all the terms, we obtain that the Frank free energy is indeed given by the expression for Ψ provided in (4.4).
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Gay-Balmaz, F., Ratiu, T.S. & Tronci, C. Euler-Poincaré Approaches to Nematodynamics. Acta Appl Math 120, 127–151 (2012). https://doi.org/10.1007/s10440-012-9719-x
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DOI: https://doi.org/10.1007/s10440-012-9719-x