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The hidden spatial geometry of non-Abelian gauge theories

The Gauss law constraint in the Hamiltonian form of the $SU(2)$ gauge theory of gluons is satisfied by any functional of the gauge invariant tensor variable $\phi^{ij} = B^{ia} B^{ja}$. Arguments are given that the tensor $G_{ij} = (\phi^{-1})_{ij}\,\det B$ is a more appropriate variable. When the H...

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Autores principales: Freedman, Daniel Z., Haagensen, Peter E., Johnson, Kenneth, Latorre, Jose I.
Lenguaje:eng
Publicado: 1993
Materias:
Acceso en línea:http://cds.cern.ch/record/253448
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author Freedman, Daniel Z.
Haagensen, Peter E.
Johnson, Kenneth
Latorre, Jose I.
author_facet Freedman, Daniel Z.
Haagensen, Peter E.
Johnson, Kenneth
Latorre, Jose I.
author_sort Freedman, Daniel Z.
collection CERN
description The Gauss law constraint in the Hamiltonian form of the $SU(2)$ gauge theory of gluons is satisfied by any functional of the gauge invariant tensor variable $\phi^{ij} = B^{ia} B^{ja}$. Arguments are given that the tensor $G_{ij} = (\phi^{-1})_{ij}\,\det B$ is a more appropriate variable. When the Hamiltonian is expressed in terms of $\phi$ or $G$, the quantity $\Gamma^i_{jk}$ appears. The gauge field Bianchi and Ricci identities yield a set of partial differential equations for $\Gamma$ in terms of $G$. One can show that $\Gamma$ is a metric-compatible connection for $G$ with torsion, and that the curvature tensor of $\Gamma$ 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 $\det G=\det B=0$. 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 $\det B=0$. 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.
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spelling cern-2534482020-07-23T02:47:57Zhttp://cds.cern.ch/record/253448engFreedman, Daniel Z.Haagensen, Peter E.Johnson, KennethLatorre, Jose I.The hidden spatial geometry of non-Abelian gauge theoriesGeneral Theoretical PhysicsParticle Physics - TheoryThe Gauss law constraint in the Hamiltonian form of the $SU(2)$ gauge theory of gluons is satisfied by any functional of the gauge invariant tensor variable $\phi^{ij} = B^{ia} B^{ja}$. Arguments are given that the tensor $G_{ij} = (\phi^{-1})_{ij}\,\det B$ is a more appropriate variable. When the Hamiltonian is expressed in terms of $\phi$ or $G$, the quantity $\Gamma^i_{jk}$ appears. The gauge field Bianchi and Ricci identities yield a set of partial differential equations for $\Gamma$ in terms of $G$. One can show that $\Gamma$ is a metric-compatible connection for $G$ with torsion, and that the curvature tensor of $\Gamma$ 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 $\det G=\det B=0$. 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 $\det B=0$. 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.The Gauss law constraint in the Hamiltonian form of the $SU(2)$ gauge theory of gluons is satisfied by any functional of the gauge invariant tensor variable $\phi~{ij} = B~{ia} B~{ja}$. Arguments are given that the tensor $G_{ij} = (\phi~{-1})_{ij}\,\det B$ is a more appropriate variable. When the Hamiltonian is expressed in terms of $\phi$ or $G$, the quantity $\Gamma~i_{jk}$ appears. The gauge field Bianchi and Ricci identities yield a set of partial differential equations for $\Gamma$ in terms of $G$. One can show that $\Gamma$ is a metric-compatible connection for $G$ with torsion, and that the curvature tensor of $\Gamma$ 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 $\det G=\det B=0$. 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 $\det B=0$. 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.hep-th/9309045MIT-CTP-2238CERN-TH-7010-93CERN-TH-7010-93CTP-2238oai:cds.cern.ch:2534481993
spellingShingle General Theoretical Physics
Particle Physics - Theory
Freedman, Daniel Z.
Haagensen, Peter E.
Johnson, Kenneth
Latorre, Jose I.
The hidden spatial geometry of non-Abelian gauge theories
title The hidden spatial geometry of non-Abelian gauge theories
title_full The hidden spatial geometry of non-Abelian gauge theories
title_fullStr The hidden spatial geometry of non-Abelian gauge theories
title_full_unstemmed The hidden spatial geometry of non-Abelian gauge theories
title_short The hidden spatial geometry of non-Abelian gauge theories
title_sort hidden spatial geometry of non-abelian gauge theories
topic General Theoretical Physics
Particle Physics - Theory
url http://cds.cern.ch/record/253448
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