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On the Green’s functions of quantized fields. I

Julian Schwinger
PNAS July 1, 1951 37 (7) 452-455; https://doi.org/10.1073/pnas.37.7.452
Julian Schwinger
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  1. Communicated May 22, 1951

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The temporal development of quantized fields, in its particle aspect, is described by propagation functions, or Green’s functions. The construction of these functions for coupled fields is usually considered from the viewpoint of perturbation theory. Although the latter may be resorted to for detailed calculations, it is desirable to avoid founding the formal theory of the Green’s functions on the restricted basis provided by the assumption of expandability in powers of coupling constants. These notes are a preliminary account of a general theory of Green’s functions, in which the defining property is taken to be the representation of the fields of prescribed sources.

We employ a quantum dynamical principle for fields which has been described elsewhere.1 This principle is a differential characterization of the function that produces a transformation from eigenvalues of a complete set of commuting operators on one space-like surface to eigenvalues of another set on a different surface,2

Embedded Image

Here ℒ is the Lagrange function operator of the system. For the example of coupled Dirac and Maxwell fields, with external sources for each field, the Lagrange function may be taken asEmbedded Imagewhich implies the equations of motionEmbedded ImagewhereEmbedded ImageWith regard to commutation relations, we need only note the anticommutativity of the source spinors with the Dirac field components.

We shall restrict our attention to changes in the transformation function that arise from variations of the external sources. In terms of the notationEmbedded Imagethe dynamical principle can then be writtenEmbedded ImagewhereEmbedded ImageThe effect of a second, independent variation is described byEmbedded Imagein which the notation ( )+ indicates temporal ordering of the operators. As examples we haveEmbedded ImageandEmbedded ImageThe latter result can be expressed in the notationEmbedded Imagealthough one may supplement the right side with an arbitrary gradient. This consequence of the charge conservation condition, ∂μJμ = 0, corresponds to the gauge invariance of the theory.

A Green’s function for the Dirac field, in the absence of an actual spinor source, is defined byEmbedded ImageAccording to ( 9), and the anticommutativity of δη(x′) with ψ(x), we haveEmbedded Imagewhere Embedded Image. On combining the differential equation for Embedded Image with ( 11), we obtain the functional differential equationEmbedded ImageAn accompanying equation for Embedded Image is obtained by noting thatEmbedded Imagein which the trace refers to the spinor indices, and an average is to be taken of the forms obtained with Embedded Image. Thus, with the special choice of gauge, Embedded Image, we haveEmbedded Image

The simultaneous equations ( 14) and ( 16) provide a rigorous description of G(x, x′) and 〈Aμ(x)〉.

A Maxwell field Green’s function is defined byEmbedded Image

The differential equations obtained from ( 16) and the gauge condition areEmbedded Image

More complicated Green’s functions can be discussed in an analogous manner. The Dirac field Green’s function defined byEmbedded Imagemay be called a “two-particle” Green’s function, as distinguished from the “one-particle” G(x, x′). It is given explicitly byEmbedded Image

This function is antisymmetrical with respect to the interchange of x1 and x2, and of x1′ and x2′ (including the suppressed spinor indices). It obeys the differential equationEmbedded Imagewhere 𝕱 is the functional differential operator of ( 14). More symmetrically written, this equation readsEmbedded Imagein which the two differential operators are commutative.

The replacement of the Dirac field by a Kemmer field involves alterations beyond those implied by the change in statistics. Not all components of the Kemmer field are dynamically independent. Thus, if 0 refers to some arbitrary time-like direction, we haveEmbedded Imagewhich is an equation of constraint expressing Embedded Image in terms of the independent field components Embedded Image, and of the external source. Accordingly, in computing Embedded Image we must take into account the change induced in Embedded Image, whenceEmbedded Image

The temporal ordering is with respect to the arbitrary time-like direction.

The Green’s function is independent of this direction, however, and satisfies equations which are of the same form as ( 14) and ( 16), save for a sign change in the last term of the latter equation which arises from the different statistics associated with the integral spin field.

References

  1. ↵
    Schwinger J., Phys. Rev., June 15, 1951 issue.
  2. ↵
    We employ units in which ħ = c = 1.
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On the Green’s functions of quantized fields. I
Julian Schwinger
Proceedings of the National Academy of Sciences Jul 1951, 37 (7) 452-455; DOI: 10.1073/pnas.37.7.452

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On the Green’s functions of quantized fields. I
Julian Schwinger
Proceedings of the National Academy of Sciences Jul 1951, 37 (7) 452-455; DOI: 10.1073/pnas.37.7.452
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