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Linearisation of the mechanical system at an equilibrium: M(q_0) xi'' + D²U(q_0) xi = 0, and the small-oscillation quadratic model

Statement

Let n≥1, let Ω⊆Rn be open, let M:Ω→Mn(R) be a C2 field of symmetric positive definite matrices, let U:Ω→R be C2, and let q0∈Ω be a mechanical equilibrium, that is ∇U(q0)=0 (The mechanical first-order field, Lagrangian and energy of a configuration-dependent kinetic metric in a chart). Let G be the mechanical vector field on Ω×Rn. Then:

  1. G is totally differentiable at (q0,0) (The total (Fréchet) derivative Df(a) as the linear first-order approximation with o(∥h∥2) remainder) and, writing D2U(q0) for the Hessian matrix (The Hessian matrix and critical points of a scalar field),

DG(q0,0)(δq,δv)=(δv, −M(q0)−1D2U(q0) δq)(δq,δv∈Rn);

  1. consequently the linearised equation at the equilibrium is

ξ′′=−M(q0)−1D2U(q0) ξ,equivalentlyM(q0)ξ′′+D2U(q0) ξ=0,

a constant-coefficient system whose mass matrix M(q0) is symmetric positive definite and whose stiffness matrix D2U(q0) is symmetric (The Hessian of a C2 scalar field is symmetric); 3. if in addition q0 is a strict local minimum of U, then K:=D2U(q0) is non-negative, so the hypotheses of Decoupling of the constant-coefficient quadratic system Mq′′+Kq=0 into normal modes, with the zero-mode and energy identities are satisfied by M(q0) and K, and the linearised system is exactly the constant-coefficient quadratic system of that theorem with mass matrix M(q0) and stiffness K; its modes are the normal modes of the linearisation.

Facts & Assumptions

Given: The C2 kinetic metric field M, the C2 potential U, the equilibrium q0, and the vector field G(q,v)=(v,H(q,v)) with H(q,v)=M(q)−1(12∇qf(q,v)−(DqM(q)[v])v−∇U(q)), f(q,v)=vTM(q)v.

[F1]

Regularity: under the stated hypotheses G is of class C1 on Ω×Rn (the inverse M(q)−1 has entries polynomial in the entries of M divided by the nonvanishing continuous function det⁡M(q)), hence totally differentiable at every point (The mechanical first-order field, Lagrangian and energy of a configuration-dependent kinetic metric in a chart, If det⁡(A) is a unit, then A−1=det⁡(A)−1adj⁡(A), If all partial derivatives exist on a neighbourhood and are continuous at a point, then the map is totally differentiable there with Jacobian derivative, Ck Euclidean maps and diffeomorphisms).

[F2]

At (q0,0): ∇qf(q0,0)=0 and its q-derivative vanishes, because ∂k(vTM(q)v)=vT∂kM(q)v is a quadratic form in v vanishing identically at v=0; similarly (DqM(q)[v])v=∑kvk∂kM(q)v is quadratic in v, so it and both of its first partial derivatives vanish at v=0 (The Jacobian matrix of partial derivatives and the gradient in the scalar-valued case, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, Rectangular matrix multiplication and the identity matrix In, including zero-sized shapes).

[F4]

At a strict local minimum, ∇U(q0)=0 and D2U(q0) is non-negative (A C² local minimum has vanishing gradient and positive semidefinite Hessian); and the constant-coefficient system Mξ′′+Kξ=0 with M symmetric positive definite and K symmetric non-negative is decoupled by Decoupling of the constant-coefficient quadratic system Mq′′+Kq=0 into normal modes, with the zero-mode and energy identities.

Proof

technique · direct; differentiate the explicit components of $G$ at the equilibrium and substitute
1.1givenF1algebra

The linearisation of G at (q0,0) is DG(q0,0)(δq,δv)=(δv, DqH(q0,0)δq+DvH(q0,0)δv). We compute the two partial derivatives of H=M−1B with B(q,v):=12∇qf(q,v)−(DqM(q)[v])v−∇U(q).

2.1step 1.1F2F3algebra

At (q0,0), B(q0,0)=12∇qf(q0,0)−0−∇U(q0)=0 by [F2] and the equilibrium condition. Hence DqH(q0,0)δq=Dq(M−1)(q0)[δq] B(q0,0)+M(q0)−1DqB(q0,0)δq=M(q0)−1DqB(q0,0)δq, and by [F2] and [F3] the derivative of B in q at (q0,0) is −12⋅0+0−D2U(q0)=−D2U(q0). Hence DqH(q0,0)=−M(q0)−1D2U(q0).

2.2step 1.12.1F2algebra

Similarly DvH(q0,0)=M(q0)−1DvB(q0,0) because B(q0,0)=0 again kills the derivative of M−1 along v; and DvB(q0,0)=0 because both 12∇qf and (DqM(q)[v])v are quadratic in v with vanishing first v-derivative at v=0 [F2]. Therefore DG(q0,0)(δq,δv)=(δv,−M(q0)−1D2U(q0)δq), which is clause 1.

2.3step 1.12.2F3algebra

Clause 2: the linearised first-order system is ξ′=η, η′=−M(q0)−1D2U(q0)ξ; eliminating η and multiplying by the invertible matrix M(q0) gives M(q0)ξ′′+D2U(q0)ξ=0. The matrix D2U(q0) is symmetric by [F3], and M(q0) is symmetric positive definite by hypothesis; the stiffness K:=D2U(q0) need not be non-negative, and no normal-mode conclusion is drawn at this point.

3.1step 2.3F4∎

Clause 3: if q0 is a strict local minimum, [F4] shows that K=D2U(q0) is non-negative; with M=M(q0) the hypotheses of the quadratic-mode theorem are exactly satisfied (symmetric positive definite mass and symmetric non-negative stiffness), and its clauses describe the normal modes of the linearisation.

Remarks

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