Inertia coefficients, moving constraints, and homogeneity identities.
Chapter 10
1. Geometry inside the kinetic energy
The term mr2θ˙2/2 in polar coordinates is not an extra interaction. It is ordinary translational kinetic energy expressed in variables whose unit displacements correspond to different physical distances. Understanding this structure explains generalized momentum, the inertial coefficients in Lagrange's equations, and the conditions under which the energy function equals T+V.
This chapter uses the chain rule and dot product from Unit 1. Coefficients may depend on coordinates and time, but are held fixed when differentiating with respect to generalized velocities.
2. Expansion into quadratic, linear, and constant parts
The vector eai describes the positional response to coordinate qi, and wa describes transport caused by the prescribed time dependence of the constraints. Squaring gives
The subscripts indicate degree in the velocities. T0 does not mean zero kinetic energy: a bead can have q˙=0 relative to a moving support while still moving in the laboratory. If the transformation has no explicit time dependence, all wa vanish and T=T2.
3. Symmetry and positivity of the inertia coefficients
Because the dot product is symmetric, Mij=Mji. For any real numbers zi,
For positive masses and regular independent coordinates, a nonzero vector z produces a nonzero displacement of at least one particle. The right-hand side is then strictly positive. Thus the matrix M is positive definite in a regular coordinate patch and invertible there.
Differentiating the quadratic expression uses its symmetry:
Hence ∂2T/∂q˙i∂q˙j=Mij. For a velocity-independent V, this is also the velocity Hessian of L. Invertibility will permit replacing velocities by momenta in Hamiltonian mechanics. A coordinate singularity, such as polar coordinates at r=0, can make this representation singular even though the Cartesian mechanics is regular.
4. Euler's identity and the energy function
A homogeneous function of degree s satisfies f(λq˙)=λsf(q˙). Differentiate both sides with respect to λ at λ=1:
For time-independent transformations, T1=T0=0 and E=T+V. Whether that quantity is conserved is a second question, decided by E˙=∑iQiq˙i−∂tL. The equality with mechanical energy and the constancy along a motion require different checks.
5. The kinetic-energy derivative identity
One further property explains why differentiating a scalar can recover the projection of acceleration. With constant masses,
This is a kinetic-energy identity, valid also for smooth explicitly time-dependent transformations. Its use to derive Lagrange's equations from D’Alembert's principle is placed in the optional appendix, respecting the syllabus distinction.
6. Applications
Example 1 · Polar kinetic energy
For x=rcosθ, y=rsinθ, one finds er=(cosθ,sinθ) and eθ=(−rsinθ,rcosθ). Their dot products are 1,0,r2. Thus Mrr=m, Mrθ=0, Mθθ=mr2, and
Here pr=mr˙ and pθ=mr2θ˙. Direct calculation gives r˙pr+θ˙pθ=mr˙2+mr2θ˙2=2T. The angular momentum coefficient is a moment of inertia, not a mass. At r=0, the angular coordinate ceases to distinguish positions.
Example 2 · A pendulum with a moving pivot
Let the pivot move horizontally along X(t). With x=X(t)+asinθ and y=−acosθ,
This differs from laboratory T+V by the linear transport term and twice the constant term. The momentum is not simply the bob's angular momentum relative to the pivot. Its extra term records the prescribed support motion in the laboratory kinetic energy.
Example 3 · A bead on a rotating radial wire
A straight horizontal wire through the origin rotates at prescribed angular speed Ω. Choose signed distance q along it, so r=(qcosΩt,qsinΩt). Then eq⋅w=0, ∣w∣2=Ω2q2, and
Lagrange's equation gives mq¨−mΩ2q=0. The energy function is E=mq˙2/2−mΩ2q2/2 and is conserved because this reduced L is autonomous. Laboratory kinetic energy is not conserved: the motor sustaining the rotation supplies work through the wire reaction. Thus autonomy of a reduced Lagrangian need not imply conservation of laboratory mechanical energy.
Example 4 · Mixed kinetic terms
Consider T=21m(q˙12+2αq˙1q˙2+q˙22), where both coordinates have dimensions of length and ∣α∣<1. The coefficient matrix is m(1αα1), with determinant m2(1−α2)>0.
The momenta are p1=m(q˙1+αq˙2) and p2=m(αq˙1+q˙2). Multiplying each by its velocity and adding gives 2T, including both cross terms. Solving the two equations gives
When α=1, only q˙1+q˙2 affects T, so the assumed two-velocity description is singular. The restriction is mathematical information about independence, not an arbitrary algebraic inconvenience.
7. Conditions behind the familiar formulas
Before writing ∑ipiq˙i=2T, check that the entire kinetic energy is quadratic homogeneous in the generalized velocities. Moving constraints can add lower-degree terms. Before replacing E by T+V, check the same condition and the absence of velocity dependence in V. These checks will be central to constructing and interpreting the Hamiltonian.