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Discrete gravity in one dimension

A model for quantum gravity in one (time) dimension is discussed, based on Regge's discrete formulation of gravity. The nature of exact continuous lattice diffeomorphisms and the implications for a regularized gravitational measure are examined. After introducing a massless scalar field coupled...

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Detalles Bibliográficos
Autores principales: Hamber, Herbert W., Williams, Ruth M.
Lenguaje:eng
Publicado: 1994
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0550-3213(95)00358-Y
http://cds.cern.ch/record/273612
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author Hamber, Herbert W.
Williams, Ruth M.
author_facet Hamber, Herbert W.
Williams, Ruth M.
author_sort Hamber, Herbert W.
collection CERN
description A model for quantum gravity in one (time) dimension is discussed, based on Regge's discrete formulation of gravity. The nature of exact continuous lattice diffeomorphisms and the implications for a regularized gravitational measure are examined. After introducing a massless scalar field coupled to the edge lengths, the scalar functional integral is performed exactly on a finite lattice, and the ensuing change in the measure is determined. It is found that the renormalization of the cosmological constant due to the scalar field fluctuations vanishes identically in one dimension. A simple decimation renormalization group transformation is performed on the partition function and the results are compared with the exact solution. Finally the properties of the spectrum of the scalar Laplacian are compared with results obtained for a Poissonian distribution of edge lengths.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1994
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spelling cern-2736122023-03-14T16:35:32Zdoi:10.1016/0550-3213(95)00358-Yhttp://cds.cern.ch/record/273612engHamber, Herbert W.Williams, Ruth M.Discrete gravity in one dimensionParticle Physics - TheoryA model for quantum gravity in one (time) dimension is discussed, based on Regge's discrete formulation of gravity. The nature of exact continuous lattice diffeomorphisms and the implications for a regularized gravitational measure are examined. After introducing a massless scalar field coupled to the edge lengths, the scalar functional integral is performed exactly on a finite lattice, and the ensuing change in the measure is determined. It is found that the renormalization of the cosmological constant due to the scalar field fluctuations vanishes identically in one dimension. A simple decimation renormalization group transformation is performed on the partition function and the results are compared with the exact solution. Finally the properties of the spectrum of the scalar Laplacian are compared with results obtained for a Poissonian distribution of edge lengths.A model for quantum gravity in one (time) dimension is discussed, based on Regge's discrete formulation of gravity. The nature of exact continuous lattice diffeomorphisms and the implications for a regularized gravitational measure are examined. After introducing a massless scalar field coupled to the edge lengths, the scalar functional integral is performed exactly on a finite lattice, and the ensuing change in the measure is determined. It is found that the renormalization of the cosmological constant due to the scalar field fluctuations vanishes identically in one dimension. A simple decimation renormalization group transformation is performed on the partition function and the results are compared with the exact solution. Finally the properties of the spectrum of the scalar Laplacian are compared with results obtained for a Poissonian distribution of edge lengths.A model for quantum gravity in one (time) dimension is discussed, based on Regge's discrete formulation of gravity. The nature of exact continuous lattice diffeomorphisms and the implications for a regularized gravitational measure are examined. After introducing a massless scalar field coupled to the edge lengths, the scalar functional integral is performed exactly on a finite lattice, and the ensuing change in the measure is determined. It is found that the renormalization of the cosmological constant due to the scalar field fluctuations vanishes identically in one dimension. A simple decimition renormalization group transformation is performed on the partition function and the results are compared with the exact solution. Finally the properties of the spectrum of the scalar Laplacian are compared with results obtained for a Poissonian distribution of edge lengths.hep-th/9412089CERN-TH-7378-94CERN-TH-7378-94oai:cds.cern.ch:2736121994-12-10
spellingShingle Particle Physics - Theory
Hamber, Herbert W.
Williams, Ruth M.
Discrete gravity in one dimension
title Discrete gravity in one dimension
title_full Discrete gravity in one dimension
title_fullStr Discrete gravity in one dimension
title_full_unstemmed Discrete gravity in one dimension
title_short Discrete gravity in one dimension
title_sort discrete gravity in one dimension
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/0550-3213(95)00358-Y
http://cds.cern.ch/record/273612
work_keys_str_mv AT hamberherbertw discretegravityinonedimension
AT williamsruthm discretegravityinonedimension