Canonical coordinates

Classical mechanics
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In mathematics and classical mechanics, canonical coordinates are sets of coordinates which can be used to describe a physical system at any given point in time (locating the system within phase space). Canonical coordinates are used in the Hamiltonian formulation of classical mechanics. A closely related concept also appears in quantum mechanics; see the Stone–von Neumann theorem and canonical commutation relations for details.

As Hamiltonian mechanics is generalized by symplectic geometry and canonical transformations are generalized by contact transformations, so the 19th century definition of canonical coordinates in classical mechanics may be generalized to a more abstract 20th century definition of coordinates on the cotangent bundle of a manifold.

Definition, in classical mechanics

In classical mechanics, canonical coordinates are coordinates $q_i\,$ and $p_i\,$ in phase space that are used in the Hamiltonian formalism. The canonical coordinates satisfy the fundamental Poisson bracket relations:

\{q_i, q_j\} = 0 \qquad \{p_i, p_j\} = 0 \qquad \{q_i, p_j\} = \delta_{ij}

A typical example of canonical coordinates is for $q_i$ to be the usual Cartesian coordinates, and $p_i$ to be the components of momentum. Hence in general, the $p_i$ coordinates are referred to as "conjugate momenta."

Canonical coordinates can be obtained from the generalized coordinates of the Lagrangian formalism by a Legendre transformation, or from another set of canonical coordinates by a canonical transformation.

Definition, on cotangent bundles

Canonical coordinates are defined as a special set of coordinates on the cotangent bundle of a manifold. They are usually written as a set of $(q^i,p_j)$ or $(x^i,p_j)$ with the x 's or q 's denoting the coordinates on the underlying manifold and the p 's denoting the conjugate momentum, which are 1-forms in the cotangent bundle at point q in the manifold.

A common definition of canonical coordinates is any set of coordinates on the cotangent bundle that allow the canonical one-form to be written in the form

\sum_i p_i\,\mathrm{d}q^i

up to a total differential. A change of coordinates that preserves this form is a canonical transformation; these are a special case of a symplectomorphism, which are essentially a change of coordinates on a symplectic manifold.

In the following exposition, we assume that the manifolds are real manifolds, so that cotangent vectors acting on tangent vectors produce real numbers.

Formal development

Given a manifold Q, a vector field X on Q (or equivalently, a section of the tangent bundle TQ) can be thought of as a function acting on the cotangent bundle, by the duality between the tangent and cotangent spaces. That is, define a function

P_X:T^*Q\to \mathbb{R}

such that

P_X(q,p)=p(X_q)

holds for all cotangent vectors p in $T_q^*Q$ . Here, $X_q$ is a vector in $T_qQ$ , the tangent space to the manifold Q at point q. The function $P_X$ is called the momentum function corresponding to X.

In local coordinates, the vector field X at point q may be written as

X_q=\sum_i X^i(q) \frac{\partial}{\partial q^i}

where the $\partial /\partial q^i$ are the coordinate frame on TQ. The conjugate momentum then has the expression

P_X(q,p)=\sum_i X^i(q) \;p_i

where the $p_i$ are defined as the momentum functions corresponding to the vectors $\partial /\partial q^i$ :

p_i = P_{\partial /\partial q^i}

The $q^i$ together with the $p_j$ together form a coordinate system on the cotangent bundle $T^*Q$ ; these coordinates are called the canonical coordinates.

Generalized coordinates

In Lagrangian mechanics, a different set of coordinates are used, called the generalized coordinates. These are commonly denoted as $(q^i,\dot{q}^i)$ with $q^i$ called the generalized position and $\dot{q}^i$ the generalized velocity. When a Hamiltonian is defined on the cotangent bundle, then the generalized coordinates are related to the canonical coordinates by means of the Hamilton–Jacobi equations.

References

Goldstein, Herbert; Poole, Charles P., Jr.; Safko, John L. (2002). Classical Mechanics (3rd ed.). San Francisco: Addison Wesley. pp. 347–349. ISBN 0-201-65702-3.

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