From NSDL Materials Digital Library Wiki
Jump to: navigation, search

The Lagrangian of a dynamical system is defined as the Kinetic Energy T minus the Potential Energy U, or

 \bold L = \bold T -\bold U .

To acquire equations of motion for a dynamical system, one simply computes the Lagrange Equation,

{\partial{L}\over \partial q_i} = {\mathrm{d} \over \mathrm{d}t}{\partial{L}\over \partial{\dot{q_i}}}.

for each generalized coordinate qi. When qi = ri (i.e. the generalized coordinates are simply the Cartesian coordinates), Lagrange's equations reduce to Newton's second law.

The n generalized coordinates are the coordinates associated with the n degrees of freedom of the system. For example,

  • The rotation angles θ1 and θ2 in a double pendulum system
  • The 3N spatial coordinates for N particles in three-dimensional space
  • The 6N spatial plus rotational coordinates for N rigid bodies in three-dimensional space
  • The θ and φ of a particle confined to the surface of a sphere
Personal tools