13.07.2015 Views

Mathematical Methods for Physics and Engineering - Matematica.NET

Mathematical Methods for Physics and Engineering - Matematica.NET

Mathematical Methods for Physics and Engineering - Matematica.NET

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

26.12 PHYSICAL APPLICATIONS OF TENSORSsection 26.7, since J <strong>and</strong> ω are vectors). The tensor is called the inertia tensor at Oof the assembly <strong>and</strong> depends only on the distribution of masses in the assembly<strong>and</strong> not upon the direction or magnitude of ω.A more realistic situation obtains if a continuous rigid body is considered. Inthis case, m (α) must be replaced everywhere by ρ(r) dx dy dz <strong>and</strong> all summationsby integrations over the volume of the body. Written out in full in Cartesians,the inertia tensor <strong>for</strong> a continuous body would have the <strong>for</strong>m⎛ ∫(y 2 + z 2 )ρdV − ∫ xyρ dV − ∫ ⎞xzρ dVI =[I ij ]= ⎝ − ∫ ∫xyρ dV (z 2 + x 2 )ρdV − ∫ yzρ dV− ∫ xzρ dV − ∫ ⎠ ,∫yzρ dV (x 2 + y 2 )ρdVwhere ρ = ρ(x, y, z) is the mass distribution <strong>and</strong> dV st<strong>and</strong>s <strong>for</strong> dx dy dz; theintegrals are to be taken over the whole body. The diagonal elements of thistensor are called the moments of inertia <strong>and</strong> the off-diagonal elements without theminus signs are known as the products of inertia.◮Show that the kinetic energy of the rotating system is given by T = 1 2 I jlω j ω l .By an argument parallel to that already made <strong>for</strong> J, the kinetic energy is given by∑T = 1 m ( (α) ṙ (α) · ṙ (α))2= 1 2= 1 2= 1 2α∑αm (α) ɛ ijk ω j x (α)kɛ ilmω l x (α)m∑m (α) (δ jl δ km − δ jm δ kl )x (α)kx(α) m ω j ω lα∑ [ (m (α) δ ) ]jl r(α) 2− x(α)x (α) ω j ω lα= 1 I 2 jlω j ω l .Alternatively, since J j = I jl ω l we may write the kinetic energy of the rotating system asT = 1 J 2 jω j . ◭The above example shows that the kinetic energy of the rotating body can beexpressed as a scalar obtained by twice contracting ω with the inertia tensor. Italso shows that the moment of inertia of the body about a line given by the unitvector ˆn is I jlˆn j ˆn l (or ˆn T Iˆn in matrix <strong>for</strong>m).Since I (≡ I jl ) is a real symmetric second-order tensor, it has associated with itthree mutually perpendicular directions that are its principal axes <strong>and</strong> have thefollowing properties (proved in chapter 8):(i) with each axis is associated a principal moment of inertia λ µ , µ =1, 2, 3;(ii) when the rotation of the body is about one of these axes, the angularvelocity <strong>and</strong> the angular momentum are parallel <strong>and</strong> given byJ = Iω = λ µ ω,i.e. ω is an eigenvector of I with eigenvalue λ µ ;951jl

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!