Class Information

Moving coordinate systems, three-body problems, partial differential equations, wave propagation (strings, membranes, fluids), boundary value problems, normal modes, fluid equations of motion, viscosity; virtual work, Lagrange’s equations, Hamilton’s equations; angular momentum of a rigid body, inertia tensor, Euler’s equations, Euler angles, tops and gyroscopes, small vibrations.

Textbook: Classical Mechanics by John Taylor

(This description is a bit outdated. The inertia tensor and other rigid body stuff like Euler angles, tops, etc. was covered in Classical Mechanics).

Mechanics in Non-Inertial Frames

For a point on a rigid body
v=ω×r

Proof

Diagram of point on rigid body
v=ω (ρsinθ)=ω×r

Example Problems

Example 1: Double Pendulum – Lagrangian Mechanics

For the first mass:
v1=ϕ1˙l1ϕ1^
T=(ϕ1˙l1)2m12
For the second mass:
v2=ϕ1˙l1ϕ1^+ϕ2˙l2ϕ2^
v22=a2+b2+2ab
v22=l12ϕ1˙2+l22ϕ2˙2+2l1l2ϕ1ϕ2(ϕ1^ϕ2^)
v22=l12ϕ1˙2+l22ϕ2˙2+2l1l2ϕ1ϕ2cos(ϕ1ϕ2)

Example 2: 7.29 From Taylor – Lagrangian Mechanics

A particle with mass m moving with fixed ω

Image of particle moving

Just use cartesian coordinates, since there is no symmetry we can take advantage of
r=xx^+yy^
x=lsinϕ+Rcosθ=lsinϕ+Rcosωt
y=lcosϕ+Rsinθ=lcosϕ+Rsinωt
vx=x^
vy=y^

v2=vx2+vy2

In the end, we have T(ϕ,t) with the other variables being constants

Example 3: Mass on Cylindrical Surface – Hamiltonian Mechanics

A bead of mass m, is constrained to move on the surface of a cone
ρ=cz
where c is a constant

See the Derivation of Velocity for Polar Coordinates
v=ρ˙ρ^+ρϕ˙ϕ^+z˙z^

Then we get
v2=z˙2+(ρϕ˙)2+ρ˙2

Note that the particle is not part of a rigid body, since it has freedom to move more freely.

There are no cross terms since z^, ϕ^,ρ^ are all orthogonal, so

ρ^ϕ^=0