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
Original language | English |
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Pages (from-to) | 044016 |
Number of pages | 1 |
Journal | Physical Review D |
Volume | 73 |
Issue number | 4 |
DOIs | |
Publication status | Published - 14 Feb 2006 |