More on ghosts in the Dvali-Gabadaze-Porrati model

Dmitry Gorbunov, Kazuya Koyama, and Sergei Sibiryakov
Phys. Rev. D 73, 044016 – Published 14 February 2006

Abstract

It is shown by an explicit calculation that the excitations about the self-accelerating cosmological solution of the Dvali-Gabadaze-Porrati model contain a ghost mode. This raises serious doubts about viability of this solution. Our analysis reveals the similarity between the quadratic theory for the perturbations around the self-accelerating universe and an Abelian gauge model with two Stückelberg fields.

  • Received 22 December 2005

DOI:https://doi.org/10.1103/PhysRevD.73.044016

©2006 American Physical Society

Authors & Affiliations

Dmitry Gorbunov1, Kazuya Koyama2, and Sergei Sibiryakov1

  • 1Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary prospect 7a, Moscow 117312, Russia
  • 2Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 2EG, United Kingdom

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Issue

Vol. 73, Iss. 4 — 15 February 2006

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