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Landau–de Gennes theory

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Through Phase transition and Gibbs free energy

Mathematical description

The NI transition is a first-order phase transition, albeit it is very weak. The order parameter is the Q tensor, which is symmetric, traceless, second-order tensor and vanishes in the isotropic liquid phase. We shall consider a uniaxial Q tensor, which is defined by

Q=S(nn−13I)

where S=S(T) is the scalar order parameter and n is the director. The Q tensor is zero in the isotropic liquid phase since the scalar order parameter S is zero, but becomes non-zero in the nematic phase.

Near the NI transition, the (Helmholtz or Gibbs) free energy density F is expanded about as

F=F0+12A(T)QijQji−13B(T)QijQjkQki+14C(T)(QijQij)2

or more compactly

F=F0+12A(T)tr(Q2)−13B(T)tr(Q3)+14C(T)[tr(Q2)]2.

Further, we can expand A(T)=a(T−T∗)+⋯, B(T)=b+⋯ and C(T)=c+⋯ with (a,b,c) being three positive constants. Now substituting the Q tensor results in

F−F0=a3(T−T∗)S2−2b27S3+c9S4.

This is minimized when

3a(T−T∗)S−bS2+2cS3=0.

The two required solutions of this equation are

Isotropic:SI=0,Nematic:SN=b4c[1+1−24acb2(T−T∗)]>0.

The NI transition temperature TNI is not simply equal to T∗ (which would be the case in second-order phase transition), but is given by

TNI=T∗+b227ac,SNI=b3c

SNI is the scalar order parameter at the transition.

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