Classical and Quantum Consistency of the DGP Model

By Alberto Nicolis, R. Rattazzi. 2004

511 citations recorded by the source corpus.

We study the Dvali-Gabadadze-Porrati model by the method of the boundary effective action. The truncation of this action to the bending mode π consistently describes physics in a wide range of regimes both at the classical and at the quantum level. The Vainshtein effect, which restores agreement with precise tests of general relativity, follows straightforwardly. We give a simple and general proof of stability, i.e. absence of ghosts in the fluctuations, valid for most of the relevant cases, like for instance the spherical source in asymptotically flat space. However we confirm that around certain interesting self-accelerating cosmological solutions there is a ghost. We consider the issue of quantum corrections. Around flat space π becomes strongly coupled below a macroscopic length of 1000 km, thus impairing the predictivity of the model. Indeed the tower of higher dimensional operators which is expected by a generic UV completion of the model limits predictivity at even larger length scales. We outline a non-generic but consistent choice of counterterms for which this disaster does not happen and for which the model remains calculable and successful in all the astrophysical situations of interest. By this choice, the extrinsic curvature Kµ� acts roughly like a dilaton field controlling the strength of the interaction and the cut-off scale at each space-time point. At the surface of Earth the cutoff is ∼ 1 cm but it is unlikely that the associated quantum effects be observable in table top experiments.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/c8bb326bc8a46a24e175e1e7491d4e4ccf7aba02

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In Astronomy and Astrophysics

  1. Lavinia Heisenberg
  2. K. Koyama
  3. Tsutomu Kobayashi
  4. Claudia de Rham
  5. F. Vernizzi
  6. D. Langlois
  7. S. Tsujikawa
  8. I. Sawicki

In Nuclear and High Energy Physics

  1. Lavinia Heisenberg
  2. Claudia de Rham
  3. K. Koyama
  4. Tsutomu Kobayashi
  5. Kurt Hinterbichler
  6. S. Tsujikawa
  7. I. Sawicki
  8. J. Khoury

In Statistical and Nonlinear Physics

  1. Claudia de Rham
  2. Lavinia Heisenberg
  3. Alberto Nicolis
  4. I. Sawicki
  5. Kurt Hinterbichler
  6. César Gómez
  7. E. Trincherini
  8. G. Dvali

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