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The inertia tensor of a finite bounded Borel measure about any point of R3

Definition

Let B(R3) be the Borel sigma-algebra of R3 (The Borel sigma-algebra of a topological space), let ν be a measure on the measurable space (R3,B(R3)) (Measures on sigma-algebras, Measure spaces) that is finite and bounded: ν(R3)<+∞ and ν(R3∖B‾R(0))=0 for some real R>0 (Open ball, closed ball and sphere in a metric space). Put m:=ν(R3)∈[0,+∞); nonnegativity follows from the definition of measure Measures on sigma-algebras. If m>0, then ν is a mass distribution in the sense of Mass distributions on R3: total mass, first moment and inertia matrix. If m=0, then for every Borel set E⊆R3 one has 0≤ν(E)≤ν(R3)=0, so ν is the zero measure. Integrals against ν are Lebesgue integrals as in Integral over a measurable subset and Integrable real and complex functions, and their integrals, defined componentwise for vector- and matrix-valued integrands. When m>0, recall that the inertia matrix of ν is

I(ν)=∫(∥ρ∥22I3−ρρT) dν(ρ)∈M3(R),

with I3 the identity matrix and entrywise integrals I(ν)jk=∫(∥ρ∥22δjk−ρjρk) dν, where ∥⋅∥2 and the matrix conventions are those of The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, The vector space Mm×n(F):=F m×n of m by n matrices over a field, with entrywise operations and Rectangular matrix multiplication and the identity matrix In, including zero-sized shapes.

Shifted integrand and inertia tensor about a point. For a∈R3 define the component functions

Ga(ρ)jk:=∥ρ−a∥22 δjk−(ρj−aj)(ρk−ak)(j,k∈{1,2,3}),

equivalently the matrix-valued function Ga(ρ)=∥ρ−a∥22I3−(ρ−a)(ρ−a)T, and define the inertia tensor of ν about a Iν(a)∈M3(R) by its entries

Iν(a)jk:=∫Ga(ρ)jk dν(ρ).

Under the Axiom of Countable Choice ACω (The Axiom of Countable Choice (ACω)) each entry is a finite real number; this is the content of Finiteness and a uniform bound for the entries of the inertia tensor about an arbitrary point ↗, which depends on this definition only for its notation. For a=0 the shifted integrand is the parent integrand ∥ρ∥22I3−ρρT. Thus Iν(0)=I(ν) when m>0; if m=0, the parent definition does not define I(ν), while the shifted integral remains defined and equals the zero matrix 03×3 for every a.

Scope. The definition names a mathematical function a↦Iν(a) from R3 to M3(R) determined by any finite bounded Borel measure ν and its coordinate origin. For the zero measure this function is identically 03×3. No physical body, unit system or measured mass is asserted. No translation identity for nonzero a is asserted here; the centred, positive-total-mass case is proved separately on this page.

Remarks

  • The measure need not be atomless. Points, curves, surfaces and volumes are all admissible: ν is an arbitrary bounded finite Borel measure, so finite sums of Dirac measures, lines and surface measures embedded in R3 and absolutely continuous volume measures are all special cases, exactly as in Mass distributions on R3: total mass, first moment and inertia matrix.

  • Translation of the point, not of the measure. The point a only shifts the reference point at which the second moments are computed; the measure and its coordinate representation are unchanged, and μ(ν) is not assumed to vanish unless a consumer states it.

Depends on

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