Lably
Skip to content

Calculus of moving surfaces

Extension of the classical tensor calculus

  • 3 min read
  • 4 chapters

Related on Lably

Through Velocity, Operator (mathematics) and Geometry


Suppose that Σt is the evolution of the surface Σ indexed by a time-like parameter t. The definitions of the surface velocity C and the operator ∇˙ are the geometric foundations of the CMS. The velocity C is the rate of deformation of the surface Σ in the instantaneous normal direction. The value of C at a point P is defined as the limit

C=limh→0Distance(P,P∗)h

where P∗ is the point on Σt+h that lies on the straight line perpendicular to Σt at point P. This definition is illustrated in the first geometric figure below. The velocity C is a signed quantity: it is positive when PP∗¯ points in the direction of the chosen normal, and negative otherwise. The relationship between Σt and C is analogous to the relationship between location and velocity in elementary calculus: knowing either quantity allows one to construct the other by differentiation or integration.

The tensorial time derivative ∇˙ for a scalar field F defined on Σt is the rate of change in F in the instantaneously normal direction:

δFδt=limh→0F(P∗)−F(P)h

This definition is also illustrated in second geometric figure.

The above definitions are geometric. In analytical settings, direct application of these definitions may not be possible. The CMS gives analytical definitions of C and ∇˙ in terms of elementary operations from calculus and differential geometry.

Analytical definitions

For analytical definitions of C and ∇˙, consider the evolution of S given by

Zi=Zi(t,S)

where Zi are general curvilinear space coordinates and Sα are the surface coordinates. By convention, tensor indices of function arguments are dropped. Thus the above equations contains S rather than Sα. The velocity object V=ViZi is defined as the partial derivative

Vi=∂Zi(t,S)∂t

The velocity C can be computed most directly by the formula

C=ViNi

where Ni are the covariant components of the normal vector N→.

Also, defining the shift tensor representation of the surface's tangent space Ziα=Sα⋅Zi and the tangent velocity as Vα=ZiαVi , then the definition of the ∇˙ derivative for an invariant F reads

∇˙F=∂F(t,S)∂t−Vα∇αF

where ∇α is the covariant derivative on S.

For tensors, an appropriate generalization is needed. The proper definition for a representative tensor Tjβiα reads

∇˙Tjβiα=∂Tjβiα∂t−Vη∇ηTjβiα+VmΓmkiTjβkα−VmΓmjkTkβiα+Γ˙ηαTjβiη−Γ˙βηTjηiα

where Γmjk are Christoffel symbols and Γ˙βα=∇βVα−CBβα is the surface's appropriate temporal symbols (Bβα is a matrix representation of the surface's curvature shape operator)

Sign in to keep reading

3 more chapters are free with a Lably account.

More in Topics in mathematics