And yet, at the fundamental level, they remind us that constraints in physics are not merely simplifications—they are active shapers of possibility. The wheel that refuses to slip, the blade that refuses to slide, the ice skater’s edge—all carve out a geometry of motion richer than any set of fixed coordinates can capture.
But nonholonomic constraints are different. They restrict the velocities of a system, not its positions, in a way that cannot be integrated into a positional constraint. The classic example? A rolling wheel without slipping. Take a skateboard. Its position in the plane is given by $(x, y)$ and its orientation by $\theta$. That’s 3 degrees of freedom. Now impose the “no lateral slip” condition: the wheel’s velocity perpendicular to its orientation must be zero.
In nonholonomic systems, we cannot. The constraints are linear in velocities, so we can use Lagrange multipliers to enforce them. But here’s the deep part: (in the ideal case). That means D’Alembert’s principle still holds—but only for virtual displacements consistent with the constraints. dynamics of nonholonomic systems
The resulting equations of motion are:
where $a^i_j$ are coefficients of the velocity constraints $\sum_j a^i_j(q) \dot{q}^j = 0$, and $\lambda_i$ are Lagrange multipliers. And yet, at the fundamental level, they remind
[ \dot{x} \sin \theta - \dot{y} \cos \theta = 0 ]
This leads to the , which differs from the standard Euler-Lagrange equations in a crucial way: the constraint forces do no work under virtual displacements, but real displacements (which must satisfy the constraints) may still lead to energy-conserving but non-integrable motion. They restrict the velocities of a system, not
This is a differential equation. Can you integrate it to find a relationship between $x, y,$ and $\theta$ alone? No. Because you can change the skateboard’s orientation without changing its position (spin in place), and you can move it along a closed loop and return to the same orientation but a different position (think parallel parking).