Canonical coordinates explained

In mathematics and classical mechanics, canonical coordinates are sets of coordinates on phase space which can be used to describe a physical system at any given point in time. 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 are 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 (the mathematical notion of phase space).

Definition in classical mechanics

In classical mechanics, canonical coordinates are coordinates

qi

and

pi

in phase space that are used in the Hamiltonian formalism. The canonical coordinates satisfy the fundamental Poisson bracket relations:

\left\{qi,qj\right\}=0    \left\{pi,pj\right\}=0    \left\{qi,pj\right\}=\deltaij

A typical example of canonical coordinates is for

qi

to be the usual Cartesian coordinates, and

pi

to be the components of momentum. Hence in general, the

pi

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

\left(qi,pj\right)

or

\left(xi,pj\right)

with the xs or qs denoting the coordinates on the underlying manifold and the ps 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

\sumi

i
p
idq

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, a vector field on (a section of the tangent bundle) 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

PX:T*Q\toR

such that

PX(q,p)=p(Xq)

holds for all cotangent vectors in

*Q
T
q
. Here,

Xq

is a vector in

TqQ

, the tangent space to the manifold at point . The function

PX

is called the momentum function corresponding to .

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

Xq=\sumiXi(q)

\partial
\partialqi

where the

\partial/\partialqi

are the coordinate frame on . The conjugate momentum then has the expression

PX(q,p)=\sumiXi(q)pi

where the

pi

are defined as the momentum functions corresponding to the vectors

\partial/\partialqi

:

pi=

P
\partial/\partialqi

The

qi

together with the

pj

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

\left(qi,

q

i\right)

with

qi

called the generalized position and
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.

See also

References