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Kinetic energy and angular momentum of a rigid placement: K=12m∥c′∥22+12ωTIω and Lc=RIω

Statement

Assume the Axiom of Countable Choice ACω (The Axiom of Countable Choice (ACω)), used only through the bound of Finiteness of the moments of a bounded finite Borel measure on R3 that makes the two integrands of clause 1 ν-integrable. Let J⊆R be an interval with at least two points, let ν be a centred mass distribution on R3 with total mass m and inertia matrix I (Mass distributions on R3: total mass, first moment and inertia matrix), let c:J→R3 and R:J→SO(3) be differentiable, and let x(t,ρ)=c(t)+R(t)ρ be the rigid placement with body angular velocity ω (Rigid placements, body and spatial angular velocity, and material velocities). For t∈J define K(t):=12∫∥∂tx(t,ρ)∥22 dν(ρ),Lc(t):=∫(x(t,ρ)−c(t))×(∂tx(t,ρ)−c′(t)) dν(ρ), the second integral read componentwise (Mass distributions on R3: total mass, first moment and inertia matrix). Then for every t∈J:

  1. ∂tx(t,ρ)=c′(t)+R(t)(ω(t)×ρ) for every ρ∈R3, and R′(t)=R(t)[ω(t)]×=[R(t)ω(t)]×R(t); moreover the two integrands displayed above are ν-integrable, so K(t) and Lc(t) are a well-defined finite real number and vector;
  2. K(t)=12m∥c′(t)∥22+12ω(t)TIω(t);
  3. Lc(t)=R(t)Iω(t).

Facts & Assumptions

Given: A centred mass distribution ν, differentiable c:J→R3 and R:J→SO(3), the rigid placement x(t,ρ)=c(t)+R(t)ρ, its body angular velocity ω with RTR′=[ω]×, and a time t∈J.

[L1]

The body angular velocity satisfies RTR′=[ω]×, hence R′=R[ω]×, and by conjugation R′=[Rω]×R as well; explicitly ω=((RTR′)32,(RTR′)13,(RTR′)21) Rigid placements, body and spatial angular velocity, and material velocities, The skew-matrix/cross-product correspondence [ω]×z=ω×z and its conjugation law R[ω]×RT=[Rω]×.

[L3]

The elements of SO(3) preserve the Euclidean inner product and norm: ⟨Ru,Rv⟩=⟨u,v⟩, so ∥Rv∥2=∥v∥2 The orthogonal group O(3) and the rotation group SO(3), The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, Real and complex inner product spaces, with the inner product linear in the first argument.

[L4]

The measure ν has finite total mass, ν(R3∖B‾R(0))=0 for some R>0, and vanishing first moment ∫ρj dν=0 for j=1,2,3; every polynomial of degree at most two in the coordinates is ν-integrable, with the bound of Finiteness of the moments of a bounded finite Borel measure on R3 (Mass distributions on R3: total mass, first moment and inertia matrix).

[L5]

The integral is linear on L1(ν) and equals the componentwise integral for vector- or matrix-valued integrands The Lebesgue integral is linear on L1(μ), Integral over a measurable subset, Integrable real and complex functions, and their integrals.

[L7]

For u,v∈R3, the cross product is bilinear, u×v is determined componentwise by (u×v)1=u2v3−u3v2 and its cyclic analogues, and ∥u×v∥22=∥u∥22∥v∥22−⟨u,v⟩2≤∥u∥22∥v∥22 The cross product in R3, The squared cross-product norm is the Gram determinant of two vectors.

Proof

technique · direct
1.1givenL1L2

By [L1], R′=R[ω]×, and [ω]×ρ=ω×ρ by [L2]; hence for every ρ the derivative of s↦x(s,ρ) at t is ∂tx(t,ρ)=c′(t)+R′(t)ρ=c′(t)+R(t)(ω(t)×ρ).

1.2givenL7algebra

For every ρ,ω one has the vector identity ρ×(ω×ρ)=(∥ρ∥22I3−ρρT)ω: for instance the first coordinate of the left side is ρ2(ω1ρ2−ω2ρ1)−ρ3(ω3ρ1−ω1ρ3)=ω1(ρ22+ρ32)−ρ1(ω2ρ2+ω3ρ3), which equals the first coordinate ∥ρ∥22ω1−ρ1⟨ρ,ω⟩ of the right side, and the second and third coordinates are the cyclic analogues.

2.1step 1.1givenL3L4L7algebra

The first integrand satisfies ∥∂tx(t,ρ)∥22≤4∥c′(t)∥22+4∥ω(t)∥22∥ρ∥22 by step 1.1, [L3] and the two elementary bounds ∥a+b∥22≤2∥a∥22+2∥b∥22 and ∥u×v∥2≤∥u∥2∥v∥2; the second integrand satisfies ∥(x−c)×(∂tx−c′)∥2≤∥ρ∥2∥ω(t)×ρ∥2≤∥ω(t)∥2∥ρ∥22 by step 1.1 and [L3]. Both are bounded on the support ball of ν by constants depending on t, so they are ν-integrable by [L4]; this is the integrability clause of the statement.

2.2step 1.1L3L7algebra

Expanding the square with bilinearity and symmetry of the inner product and using [L3], ∥∂tx∥22=∥c′∥22+2⟨c′,R(ω×ρ)⟩+∥ω×ρ∥22.

2.3step 1.1L2algebra

By step 1.1 the relative velocity is (x−c)′=∂tx−c′=R(ω×ρ), so the angular-momentum integrand is (x−c)×(x−c)′=Rρ×R(ω×ρ)=R(ρ×(ω×ρ)) by [L2].

3.1step 2.12.2givenL4L5L6algebra

Integrating step 2.2 with [L5] and pulling the constant R(t) and the linear map ρ↦ω×ρ through the integral, ∫∥∂tx∥22 dν=m∥c′∥22+2⟨c′,R(ω×∫ρ dν)⟩+∫∥ω×ρ∥22 dν. The middle term vanishes because ∫ρ dν=0 by [L4], and the last term equals ωTIω by [L6]; substituting into the definition of K gives clause 2.

4.1step 2.31.2givenL4L5∎

Integrating step 2.3 and substituting step 1.2, Lc(t)=R(t)∫(∥ρ∥22I3−ρρT)dν ω(t)=R(t)Iω(t), the constant matrix R(t) and the finite sum of integrals being interchanged by [L5] componentwise, and the last equality being the definition of I in Mass distributions on R3: total mass, first moment and inertia matrix. This is clause 3.

Depends on

Dependency tree · 2 levels

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