Abstract
In this paper, we study the Cauchy problem of the Poiseuille flow of the full Ericksen–Leslie model for nematic liquid crystals. The model is a coupled system of a parabolic equation for the velocity and a quasilinear wave equation for the director. For a particular choice of several physical parameter values, we construct solutions with smooth initial data and finite energy that produce, in finite time, cusp singularities—blowups of gradients. The formation of cusp singularity is due to local interactions of wave-like characteristics of solutions, which is different from the mechanism of finite time singularity formations for the parabolic Ericksen–Leslie system. The finite time singularity formation for the physical model might raise some concerns for purposes of applications. This is, however, resolved satisfactorily; more precisely, we are able to establish the global existence of weak solutions that are Hölder continuous and have bounded energy. One major contribution of this paper is our identification of the effect of the flux density of the velocity on the director and the reveal of a singularity cancellation—the flux density remains bounded while its two components approach infinity at formations of cusp singularities.
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Acknowledgements
G. Chen’s research is partially supported by NSF grant DMS-1715012, T. Huang’s research is partially supported by NSFC Grant 11601333 and Shanghai NSF Grant 16ZR1423800, and W. Liu’s research is partially supported by Simons Foundation Mathematics and Physical Sciences-Collaboration Grants for Mathematicians #581822.
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Appendix A
Appendix A
1.1 A.1. Derivation of System (2.1)
We consider the following form of solutions to the system (1.10)
It is easy to see that \(\nabla \cdot \mathbf{u}(x,t)=0 \), and \(\mathbf{u}\cdot \nabla \mathbf{u}=\mathbf{u}\cdot \nabla \mathbf{n}=\mathbf{u}\cdot \nabla \dot{\mathbf{n}}=0\). Direct computation implies
Then
and also
Hence
Since the last term in Oseen-Frank energy density is null Lagrangian term, without loss of generalization, we only compute the first three terms. The Oseen-Frank energy density of this case will be
where \(\mathbf{n}^i\) is the i-th component of \(\mathbf{n}\). Thus
The Lagrangian constant is
We are ready to derive the system (2.1). We first work on the equation of \(\theta \). By the third equation of (1.10), we have
Then
Here the vector \({\mathbf {T}}_1\) is given by
The nonzero components of vector \({\mathbf {T}}_2\) is given by
so the vector \({\mathbf {T}}_2\) is
Similarly, the vector \({\mathbf {T}}_3\) is
Plugging (A.2), (A.3) and (A.4) into (A.1), we obtain
which is exactly the second equation in (2.1).
For the equation of u, direct computation gives
and
Therefore the first equation of system (1.10) can be written into following three equations:
By these equations, one can obtain that \(P_z=a\) for some constant a. The right hand side of (A.7) can be rewritten as \((g(\theta )u_x+h(\theta )\theta _t)_x\) where \(g(\theta )\) and \(h(\theta )\) is defined as (2.2). Therefore, we obtain the first equation of (2.1).
1.2 A.2. Derivation of System (5.9)
We will in fact derive the semilinear system in XY-coordinates for (2.1) with \(\nu =\rho =1\) and \(a=0\). Recall, from (5.5) and (5.6), that we have introduced
It is easy to have that
Denote
By (4.2), we have
so
Hence,
Similarly,
On the other hand, using \(X_t-cX_x=0\), we have
Then
Similarly, we have
In summary, we have the following system of equations:
where recall that \(U=h(\theta )u_x.\)
Denote \(J=g(\theta )u_x+h(\theta )\theta _t\). Then
In terms of the variable J, the above system is
where the coefficient \(\frac{h^2(\theta )}{g(\theta )}-\gamma _1<0\) by (2.11).
For the special case where \(\gamma _1=2\), \(\gamma _2=0\) and \(g(\theta )=h(\theta )=1\), system (A.10) reduces to system (5.9).
1.3 A.3. Hölder Continuity of \({\mathcal {M}}(J)\) in §6.3
First, we consider three types of integrals in the definition of J in (6.31):
We first prove the following lemma, working generally:
Lemma A.1
If \(f(x,t)\in L^{\infty }([0,T], L^2(\mathbb {R}))\), \(g(x,t)\in L^{\infty }([0,T], L^1(\mathbb {R}))\) or \(g(x,t)\in L^{\infty }([0,T], L^2(\mathbb {R}))\) we have \(L_j(x,t)\) is Hölder continuous w.r.t x and t, for all \(j=i,ii,iii\), with exponent \(\beta \in (0,\frac{1}{4})\).
Proof
We only provide the proof of Hölder continuity w.r.t x for \(L_{iii}\), the rest cases can be proved similarly. For any \(x_1<x_2\), it is sufficient to show that
for some \(\beta \in (0,1)\). Since
The integral related to the first term \(I_1\) can be estimated as follows:
By the same argument in (3.9), and choosing \(0<\beta <\frac{1}{8}\), the first term in (A.12) should be controlled by
For the second term in (A.12),
where \(x_1-y=u\sqrt{t-s}\), and
Putting (A.13) and (A.14) into (A.12), it holds that
On the other hand, by the mean value theorem, there exists a \(\xi \in (x_1,x_2)\) such that
Hence, for the term related to \(I_2\), it holds that
The second term is similar to (3.9) and (A.13):
For the first term, one has
Let \(x_2-y=\sqrt{t-s}u\). Then it holds that
It is easy to see that
Hence,
and
Putting (A.20) and (A.21) into (A.19), we obtain
Combining (A.22) with (A.17) and (A.18), we have
It is easy to see that (A.15) and (A.23) imply (A.24).
Similarly, we can show the Hölder continuity of for \(L_{iii}\) in t , and
The proof of Hölder continuity for other terms is similar, and all bounds include a factor \(t^{\frac{1}{4}-\beta }\). \(\square \)
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Chen, G., Huang, T. & Liu, W. Poiseuille Flow of Nematic Liquid Crystals via the Full Ericksen–Leslie Model. Arch Rational Mech Anal 236, 839–891 (2020). https://doi.org/10.1007/s00205-019-01484-4
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DOI: https://doi.org/10.1007/s00205-019-01484-4