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Strong Interactions and Stability in the DGP Model

The model of Dvali, Gabadadze, and Porrati (DGP) gives a simple geometrical setup in which gravity becomes 5-dimensional at distances larger than a length scale \lambda_{DGP}. We show that this theory has strong interactions at a length scale \lambda_3 ~ (\lambda_{DGP}^2 / M_P)^{1/3}. If \lambda_{DG...

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Detalles Bibliográficos
Autores principales: Luty, M A, Porrati, Massimo, Rattazzi, Riccardo
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2003/09/029
http://cds.cern.ch/record/608903
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author Luty, M A
Porrati, Massimo
Rattazzi, Riccardo
author_facet Luty, M A
Porrati, Massimo
Rattazzi, Riccardo
author_sort Luty, M A
collection CERN
description The model of Dvali, Gabadadze, and Porrati (DGP) gives a simple geometrical setup in which gravity becomes 5-dimensional at distances larger than a length scale \lambda_{DGP}. We show that this theory has strong interactions at a length scale \lambda_3 ~ (\lambda_{DGP}^2 / M_P)^{1/3}. If \lambda_{DGP} is of order the Hubble length, then the theory loses predictivity at distances shorter than \lambda_3 ~ 1000 km. The strong interaction can be viewed as arising from a longitudinal `eaten Goldstone' mode that gets a small kinetic term only from mixing with transverse graviton polarizations, analogous to the case of massive gravity. We also present a negative-energy classical solution, which can be avoided by cutting off the theory at the same scale scale \lambda_3. Finally, we examine the dynamics of the longitudinal Goldstone mode when the background geometry is curved.
id cern-608903
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
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spelling cern-6089032019-09-30T06:29:59Zdoi:10.1088/1126-6708/2003/09/029http://cds.cern.ch/record/608903engLuty, M APorrati, MassimoRattazzi, RiccardoStrong Interactions and Stability in the DGP ModelParticle Physics - TheoryThe model of Dvali, Gabadadze, and Porrati (DGP) gives a simple geometrical setup in which gravity becomes 5-dimensional at distances larger than a length scale \lambda_{DGP}. We show that this theory has strong interactions at a length scale \lambda_3 ~ (\lambda_{DGP}^2 / M_P)^{1/3}. If \lambda_{DGP} is of order the Hubble length, then the theory loses predictivity at distances shorter than \lambda_3 ~ 1000 km. The strong interaction can be viewed as arising from a longitudinal `eaten Goldstone' mode that gets a small kinetic term only from mixing with transverse graviton polarizations, analogous to the case of massive gravity. We also present a negative-energy classical solution, which can be avoided by cutting off the theory at the same scale scale \lambda_3. Finally, we examine the dynamics of the longitudinal Goldstone mode when the background geometry is curved.hep-th/0303116CERN-TH-2003-044UMD-PP-2003-041oai:cds.cern.ch:6089032003-03-12
spellingShingle Particle Physics - Theory
Luty, M A
Porrati, Massimo
Rattazzi, Riccardo
Strong Interactions and Stability in the DGP Model
title Strong Interactions and Stability in the DGP Model
title_full Strong Interactions and Stability in the DGP Model
title_fullStr Strong Interactions and Stability in the DGP Model
title_full_unstemmed Strong Interactions and Stability in the DGP Model
title_short Strong Interactions and Stability in the DGP Model
title_sort strong interactions and stability in the dgp model
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1126-6708/2003/09/029
http://cds.cern.ch/record/608903
work_keys_str_mv AT lutyma stronginteractionsandstabilityinthedgpmodel
AT porratimassimo stronginteractionsandstabilityinthedgpmodel
AT rattazziriccardo stronginteractionsandstabilityinthedgpmodel