time dilatation of a volume element
Introduction
The rate of change of a volume element constitutes an important subject in certain applications related to the velocity field in fluid flow and elasticity,
besides it admits some physical interpretations intimately entailed to
tensor invariants
, as we shall see.
Formulae derivation
Let Xα and xi be material and spatial coordinates, respectively. Consider diffeomorphic the mapping 11See motion of continuum
Xα↦xi(Xα,τ),t0≤τ≤t, |
which represents the motion of continuum ℜ⊂(ℝ3,∥⋅∥) . The Jacobian J=|xi,α| (comma denoting partial differentiation with respect to the indicated coordinate
) of coordinate transformation
is given by
J=ϵαβγx1,αx2,βx3,γ≡Cγ3x3,γ, |
ϵαβγ being the Levi-Civita density, Cγ3 the cofactor of x3,γ in the determinant
expansion and it comes expressed as
Cγ3=ϵαβγx1,αx2,β=12(ϵαβγx1,αx2,β+ϵβαγx1,βx2,α) |
=12ϵαβγ(x1,αx2,β-x1,βx2,α)=12ϵαβγϵij3xi,αxj,β. |
So that, for any arbitrary cofactor Cγk,
Cγk=12ϵαβγϵijkxi,αxj,β. |
Let us multiply by xn,γ.
Cγkxn,γ=12ϵijkϵαβγxi,αxj,βxn,γ=12|xi,α|ϵijkϵijn=Jδnk,CγkJxn,γ=δnk, | (1) |
where we have used well-known alternator’s properties. Moreover, since the cofactor Cγk is independent on xk,γ by its own definition,
∂∂xn,γ(Jδnk)=∂J∂xk,γ=Cγk. | (2) |
But
Xγ,kxn,γ=δnk, |
which it is compared with Eq.(1) to obtain
Xγ,k=CγkJ,Cγk=JXγ,k. |
So from Eq.(2) we get
∂J∂xk,γ=JXγ,k. | (3) |
Let us now consider the relation dv=JdV between the spatial and material volume elements, and by taking the material time derivative
˙¯dv=˙JdV, | (4) |
because ˙¯dV=0, by definition. From Eqs.(3)-(4),
˙¯(dvdV)=∂J∂xi,α˙¯xi,α=∂J∂xi,α˙xi,α=JXα,ivi,α=Jvi,i |
where ˙xi,α≡vi,α are material gradient components of velocity field, thus arriving to the result due to Euler[1]
˙JJ=vi,i≡∇x⋅𝐯,˙¯logJ=∇x⋅𝐯, | (5) |
expressing the spatial divergence of velocity field.
Also, by substituting dV=dv/J in Eq.(4) we get
˙¯logdv=∇x⋅𝐯. | (6) |
Physical interpretations
-
•
The time logarithm of dilatation and the first invariant I∇x𝐯 associate to the tensor of velocity spatial gradient, coincide exactly.
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•
If we consider the Lagrangian strain tensor Eij=1/2(ui,j+uj,i+ui,kuk,j) (large strain) for ``small" strain, i.e. the initial undistorsioned (material) reference configuration
χϰ(Xi,t0) maps to near distorsioned (spatial) reference configuration χϰ+Δϰ(Xi,τ) (as τ→t0) during the motion of continuum ℜ, coinciding approximately the spatial coordinates with the material coordinates and therefore, as a consequence, the quadratic displacement gradient ui,kuk,j≈0. 22Indeed for small strain is required that ∇X𝐮⋅𝐮∇X≈𝟎 and ∇X𝐮⋅∇x𝐮≈𝟎. To see this, we consider the coordinates transformation 𝐱(τ)=χ(𝐗,τ), as τ→t0. So d𝐱=d𝐗⋅∇X𝐱. But d𝐮=d𝐗⋅∇X𝐮=d𝐱⋅∇x𝐮, then by the first equation, we have d𝐮=(d𝐗⋅∇X𝐱)⋅∇x𝐮=d𝐗⋅(∇X𝐱⋅∇x𝐮), and since d𝐗 is arbitrary ∇X𝐮=∇X𝐱⋅∇x𝐮. (The chain rule
!) Recalling now 𝐱=𝐗+𝐮, we get ∇X𝐮=[∇X(𝐗+𝐮)]⋅∇x𝐮=(𝟏+∇X𝐮)⋅∇x𝐮=∇x𝐮+∇X𝐮⋅∇x𝐮, which shows that quadratic gradient is approximately equal to zero whenever ∇X𝐮≈∇x𝐮, i.e. the material undistorsioned reference configuration ϰ be approximately equal to the spatial distorsioned configuration ϰ+Δϰ. In fact elasticity theory defines infinitesimal
strain tensor as eij≡ 1/2(ui,j+uj,i), i.e. eij≈Eij for small strain, but the definition of tensor 𝐞 is exact. So, in the vector displacement ui=xi-Xi, we take the material rate ˙ui=˙xi≡vi and hence ˙ui,j=vi,j. Therefore, according to the mentioned approximation, the material time derivative for tensors 𝐄 and 𝐞 are given by ˙Eij≈˙eij≈1/2(vi,j+vj,i). 33The last approximation because the tensors 𝐄 and 𝐞 are usually defined with respect to material coordinates and not with respect to the spatial ones. Now by contracting j=i, we get ˙Eii≈˙ei,i≈vi,i=∇⋅𝐯. 44Notice that although this is an approximated result, Eqs.(5)-(6) are exact.
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•
Considering the infinitesimal strain tensor 𝐞 (or 𝐄 for small strain), we see that sum of normal strain eii=e11+e22+e33=u1,1+u2,2+u3,3 represents the trace or first invariant I𝐞. Thus, in the initial undistorsioned reference configuration ϰ, we can use principal centered axes (i.e. along the eigenvectors
of tensor 𝐞, whose representation corresponds to pure normal strains) of a volume element dV in order to measure the induced dilatation (dv-dV)/dV in the distorsioned reference configuration ϰ+Δϰ. So, for an elemental rectangular parallelopiped of volume dV, we have
(dvdV)≈(1+e11)(1+e22)(1+e33)=1+eii+o(e2nn). (nnotsummed) By taking now the material time derivative,
˙¯(dvdV)≈˙eii≈˙Eii≈˙ui,i=˙xi,i=vi,i=∇⋅𝐯, thus completing the aimed physical interpretation.
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•
A volume-preserving motion is said to be isochoric. Then
J=|∂xi∂Xα|=1,divx𝐯=0. V is called material volume and v is called control volume.
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•
Although we have used Cartesian rectangular systems, if we introduce generalizated tensors, all the results obtained are also valid for curvilinear coordinates . For instance,
-
(a)
Divergence
∇x⋅𝐯=𝐠i⋅∂∂xi(vj𝐠j)=𝐠i⋅𝐠jvj|i=vi|i=vi,i+Γjjivi, Γjji=12g∂g∂xi,g=|gij|,gjkgki=δij, where vj|i,𝐠i,𝐠j, stand for covariant derivative
and contravariant and covariant spatial base vectors, respectively.
-
(b)
Gradient
∇X𝐮=𝐆α∂∂Xα(uβ𝐆β)=uβ|α𝐆α𝐆β=(uβ,α+Γβγαuγ)𝐆α𝐆β, Γβγα=GβδΓγαδ,Γγαδ=12(Gγδ,α+Gαδ,γ-Gγα,δ). 𝐮∇X=∂∂Xβ(uα𝐆α)𝐆β=uα|β𝐆α𝐆β=(uα,β+Γαγβuγ)𝐆α𝐆β, where 𝐆α,𝐆β are the covariant and contravariant material base vectors, respectively. mutatis mutandis for spatial gradient tensors ∇x𝐮,𝐮∇x.
-
(c)
Material time derivative
˙𝐯=˙¯vi𝐠i=∂vi∂t𝐠i+vi|jvj𝐠i=∂vi∂t𝐠i+(vi,jvj+Γikjvkvj)𝐠i, where the local time derivative
by definition.
-
(a)
References
- 1 L. Euler, Principes généraux du mouvement des fluides, Hist. Acad. Berlin 1755, 274-315, 1757.
Title | time dilatation of a volume element |
---|---|
Canonical name | TimeDilatationOfAVolumeElement |
Date of creation | 2013-03-22 15:54:28 |
Last modified on | 2013-03-22 15:54:28 |
Owner | perucho (2192) |
Last modified by | perucho (2192) |
Numerical id | 10 |
Author | perucho (2192) |
Entry type | Definition |
Classification | msc 53A45 |