Covariant classical field theory

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In mathematical physics, covariant classical field theory represents classical fields by sections of fiber bundles, and their dynamics is phrased in the context of a finite-dimensional space of fields. Nowadays, it is well known that[citation needed] jet bundles and the variational bicomplex are the correct domain for such a description. The Hamiltonian variant of covariant classical field theory is the covariant Hamiltonian field theory where momenta correspond to derivatives of field variables with respect to all world coordinates. Non-autonomous mechanics is formulated as covariant classical field theory on fiber bundles over the time axis .

Uncoupled theories

Many important examples of classical field theories which are of interest in quantum field theory are given below. In particular, these are the theories which make up the Standard Model of particle physics. These examples will be used in the discussion of the general mathematical formulation of classical field theory.

Coupled theories

Requisite mathematical structures

In order to formulate a classical field theory, the following structures are needed:

Spacetime

A smooth manifold .

This is variously known as the world manifold (for emphasizing the manifold without additional structures such as a metric), spacetime (when equipped with a Lorentzian metric), or the base manifold for a more geometrical viewpoint.

Structures on spacetime

The spacetime often comes with additional structure. Examples are

  • Metric: a (pseudo-)Riemannian metric on .
  • Metric up to conformal equivalence

as well as the required structure of an orientation, needed for a notion of integration over all of the manifold .

Symmetries of spacetime

The spacetime may admit symmetries. For example, if it is equipped with a metric , these are the isometries of , generated by the Killing vector fields. The symmetries form a group , the automorphisms of spacetime. In this case the fields of the theory should transform in a representation of .

For example, for Minkowski space, the symmetries are the Poincaré group .

Gauge, principal bundles and connections

A Lie group describing the (continuous) symmetries of internal degrees of freedom. This is referred to as the gauge group. The corresponding Lie algebra through the Lie group–Lie algebra correspondence is denoted .

A principal -bundle , otherwise known as a -torsor. This is sometimes written as

where is the canonical projection map on and is the base manifold.

Connections and gauge fields

Here we take the view of the connection as a principal connection. In field theory this connection is also viewed as a covariant derivative whose action on various fields is defined later.

A principal connection denoted is a -valued 1-form on P satisfying technical conditions of 'projection' and 'right-equivariance': details found in the principal connection article.

Under a trivialization this can be written as a local gauge field , a -valued 1-form on a trivialization patch . It is this local form of the connection which is identified with gauge fields in physics. When the base manifold is flat, there are simplifications which remove this subtlety.

Associated vector bundles and matter content

An associated vector bundle associated to the principal bundle through a representation

For completeness, given a representation , the fiber of is .

A field or matter field is a section of an associated vector bundle. The collection of these, together with gauge fields, is the matter content of the theory.

Lagrangian

A Lagrangian : given a fiber bundle , the Lagrangian is a function .

Suppose that the matter content is given by sections of with fibre from above. Then for example, more concretely we may consider to be a bundle where the fibre at is . This then allows to be viewed as a functional of a field.

This completes the mathematical prerequisites for a large number of interesting theories, including those given in the examples section above.

Theories on flat spacetime

See also

References

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