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The Hidden Spatial Geometry of Non-Abelian Gauge Theories

Abstract

The Gauss law constraint in the Hamiltonian form of the SU(2)SU(2) gauge theory of gluons is satisfied by any functional of the gauge invariant tensor variable Ο•ij=BiaBja\phi^{ij} = B^{ia} B^{ja}. Arguments are given that the tensor Gij=(Ο•βˆ’1)ij det⁑BG_{ij} = (\phi^{-1})_{ij}\,\det B is a more appropriate variable. When the Hamiltonian is expressed in terms of Ο•\phi or GG, the quantity Ξ“jki\Gamma^i_{jk} appears. The gauge field Bianchi and Ricci identities yield a set of partial differential equations for Ξ“\Gamma in terms of GG. One can show that Ξ“\Gamma is a metric-compatible connection for GG with torsion, and that the curvature tensor of Ξ“\Gamma is that of an Einstein space. A curious 3-dimensional spatial geometry thus underlies the gauge-invariant configuration space of the theory, although the Hamiltonian is not invariant under spatial coordinate transformations. Spatial derivative terms in the energy density are singular when det⁑G=det⁑B=0\det G=\det B=0. These singularities are the analogue of the centrifugal barrier of quantum mechanics, and physical wave-functionals are forced to vanish in a certain manner near det⁑B=0\det B=0. It is argued that such barriers are an inevitable result of the projection on the gauge-invariant subspace of the Hilbert space, and that the barriers are a conspicuous way in which non-abelian gauge theories differ from scalar field theories.Comment: 19 pages, TeX, CTP #223

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