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DGP Specteroscopy

Christos Charmousis, Ruth Gregory, Nemanja Kaloper, Antonio Padilla

TL;DR

This work analyzes gravitational perturbations in codimension-1 DGP braneworlds, revealing a 4D ghost on the self-accelerating branch for all brane tensions and a ghost-free normal branch. Through mode expansion, boundary-value analysis, and an effective 4D action, it identifies the ghost as the helicity-0 component of a localized light graviton (or its radion mix) in the self-accelerating background, with a milder tachyonic instability arising from a scalar mode and from Z2-breaking perturbations. The study also demonstrates that non-normalizable bulk modes and nonlocal boundary conditions can induce ghost-like behaviors, challenging the viability of self-acceleration as a gravity-driven explanation for cosmic acceleration. Conversely, the normal branch remains perturbatively ghost-free and offers a robust framework for IR modifications of gravity, while shock-wave analyses highlight IR nonlocalities and their potential implications for brane dynamics.

Abstract

We systematically explore the spectrum of gravitational perturbations in codimension-1 DGP braneworlds, and find a 4D ghost on the self-accelerating branch of solutions. The ghost appears for any value of the brane tension, although depending on the sign of the tension it is either the helicity-0 component of the lightest localized massive tensor of mass $0<m^2 < 2H^2$ for positive tension, the scalar `radion' for negative tension, or their admixture for vanishing tension. Because the ghost is gravitationally coupled to the brane-localized matter, the self-accelerating solutions are not a reliable benchmark for cosmic acceleration driven by gravity modified in the IR. In contrast, the normal branch of solutions is ghost-free, and so these solutions are perturbatively safe at large distance scales. We further find that when the $\mathbb{Z}_2$ orbifold symmetry is broken, new tachyonic instabilities, which are much milder than the ghosts, appear on the self-accelerating branch. Finally, using exact gravitational shock waves we analyze what happens if we relax boundary conditions at infinity. We find that non-normalizable bulk modes, if interpreted as 4D phenomena, may open the door to new ghost-like excitations.

DGP Specteroscopy

TL;DR

This work analyzes gravitational perturbations in codimension-1 DGP braneworlds, revealing a 4D ghost on the self-accelerating branch for all brane tensions and a ghost-free normal branch. Through mode expansion, boundary-value analysis, and an effective 4D action, it identifies the ghost as the helicity-0 component of a localized light graviton (or its radion mix) in the self-accelerating background, with a milder tachyonic instability arising from a scalar mode and from Z2-breaking perturbations. The study also demonstrates that non-normalizable bulk modes and nonlocal boundary conditions can induce ghost-like behaviors, challenging the viability of self-acceleration as a gravity-driven explanation for cosmic acceleration. Conversely, the normal branch remains perturbatively ghost-free and offers a robust framework for IR modifications of gravity, while shock-wave analyses highlight IR nonlocalities and their potential implications for brane dynamics.

Abstract

We systematically explore the spectrum of gravitational perturbations in codimension-1 DGP braneworlds, and find a 4D ghost on the self-accelerating branch of solutions. The ghost appears for any value of the brane tension, although depending on the sign of the tension it is either the helicity-0 component of the lightest localized massive tensor of mass for positive tension, the scalar `radion' for negative tension, or their admixture for vanishing tension. Because the ghost is gravitationally coupled to the brane-localized matter, the self-accelerating solutions are not a reliable benchmark for cosmic acceleration driven by gravity modified in the IR. In contrast, the normal branch of solutions is ghost-free, and so these solutions are perturbatively safe at large distance scales. We further find that when the orbifold symmetry is broken, new tachyonic instabilities, which are much milder than the ghosts, appear on the self-accelerating branch. Finally, using exact gravitational shock waves we analyze what happens if we relax boundary conditions at infinity. We find that non-normalizable bulk modes, if interpreted as 4D phenomena, may open the door to new ghost-like excitations.

Paper Structure

This paper contains 14 sections, 122 equations.