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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...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
1993
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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. |
id | cern-253448 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1993 |
record_format | invenio |
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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