Generalized coordinates simplify complex systems by reducing variables and incorporating constraints. They're crucial for describing system configurations and formulating equations of motion in classical mechanics, whether using Cartesian, polar, or angular coordinates.
Constraints play a key role in shaping system behavior. Holonomic constraints involve only coordinates and time, while non-holonomic constraints include velocities. Lagrange multipliers help incorporate these constraints into equations of motion, allowing for easier analysis of constrained systems.
Generalized Coordinates and System Constraints
Role of generalized coordinates
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Generalized coordinates
Independent variables fully describe system configuration [ q i ] ( h t t p s : / / w w w . f i v e a b l e K e y T e r m : q i ) [q_i](https://www.fiveableKeyTerm:q_i) [ q i ] ( h ttp s : // www . f i v e ab l eKey T er m : q i ) where i = 1 , 2 , . . . , n i = 1, 2, ..., n i = 1 , 2 , ... , n
Number of coordinates equals degrees of freedom
Simplify complex systems
Reduce variables needed to describe system
Automatically incorporate certain constraints
Facilitate easier formulation of equations of motion
Examples
Cartesian coordinates ( x , y , z ) (x, y, z) ( x , y , z )
Polar coordinates ( r , θ ) (r, \theta) ( r , θ )
Angular coordinates for rotational systems (pitch, yaw, roll)
Holonomic vs non-holonomic constraints
Holonomic constraints
Expressed as equations involving only coordinates and time f ( q 1 , q 2 , . . . , q n , t ) = 0 f(q_1, q_2, ..., q_n, t) = 0 f ( q 1 , q 2 , ... , q n , t ) = 0
Fixed length pendulum, bead on a wire
Non-holonomic constraints
Cannot be expressed solely in terms of coordinates and time
Involve velocities or differentials of coordinates
Rolling without slipping, knife-edge constraint
Scleronomic constraints
Time-independent (fixed-length rod)
Rheonomic constraints
Time-dependent (piston-cylinder system)
Expression of constraints
Lagrange multipliers
Additional variables λ j \lambda_j λ j incorporate constraints
Treat constrained systems as unconstrained
Constraint equations
Express holonomic constraints f j ( q 1 , q 2 , . . . , q n , t ) = 0 f_j(q_1, q_2, ..., q_n, t) = 0 f j ( q 1 , q 2 , ... , q n , t ) = 0
Augmented Lagrangian
L ∗ = L + ∑ j λ j f j ( q 1 , q 2 , . . . , q n , t ) L^* = L + \sum_j \lambda_j f_j(q_1, q_2, ..., q_n, t) L ∗ = L + ∑ j λ j f j ( q 1 , q 2 , ... , q n , t )
L L L represents original system Lagrangian
Virtual work of constraint forces
δ W c = − ∑ j λ j δ f j \delta W_c = -\sum_j \lambda_j \delta f_j δ W c = − ∑ j λ j δ f j
Equations of motion derivation
Lagrange's equations of motion
d d t ( ∂ L ∂ q i ˙ ) − ∂ L ∂ q i = Q i \frac{d}{dt}\left(\frac{\partial L}{\partial \dot{q_i}}\right) - \frac{\partial L}{\partial q_i} = Q_i d t d ( ∂ q i ˙ ∂ L ) − ∂ q i ∂ L = Q i
Q i Q_i Q i represents generalized forces (gravity, friction)
Equations of motion with constraints
d d t ( ∂ L ∗ ∂ q i ˙ ) − ∂ L ∗ ∂ q i = 0 \frac{d}{dt}\left(\frac{\partial L^*}{\partial \dot{q_i}}\right) - \frac{\partial L^*}{\partial q_i} = 0 d t d ( ∂ q i ˙ ∂ L ∗ ) − ∂ q i ∂ L ∗ = 0
Derivation steps
Express kinetic and potential energies using generalized coordinates
Form Lagrangian L = T − V L = T - V L = T − V
Add constraint terms to create augmented Lagrangian L ∗ L^* L ∗
Apply Lagrange's equations to L ∗ L^* L ∗
Solve resulting system
Equations of motion for generalized coordinates
Constraint equations (ensure system consistency)