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Probing Newton’s constant on vast scales: Dvali-Gabadadze-Porrati gravity, cosmic acceleration, and large scale structure
Author(s) -
Arthur Lue,
Román Scoccimarro,
Glenn D. Starkman
Publication year - 2004
Publication title -
physical review. d. particles, fields, gravitation, and cosmology/physical review. d, particles, fields, gravitation, and cosmology
Language(s) - English
Resource type - Journals
eISSN - 1550-7998
pISSN - 1550-2368
DOI - 10.1103/physrevd.69.124015
Subject(s) - physics , dark energy , gravitation , acceleration , classical mechanics , cosmological constant , cosmic cancer database , gravitational acceleration , theoretical physics , astrophysics , cosmology
The nature of the fuel that drives today's cosmic acceleration is an open andtantalizing mystery. The braneworld theory of Dvali, Gabadadze, and Porrati(DGP) provides a context where late-time acceleration is driven not by someenergy-momentum component (dark energy), but rather is the manifestation of theexcruciatingly slow leakage of gravity off our four-dimensional world into anextra dimension. At the same time, DGP gravity alters the gravitational forcelaw in a specific and dramatic way at cosmologically accessible scales. Wederive the DGP gravitational force law in a cosmological setting for sphericalperturbations at subhorizon scales and compute the growth of large-scalestructure. We find that a residual repulsive force at large distances givesrise to a suppression of the growth of density and velocity perturbations.Explaining the cosmic acceleration in this framework leads to a present dayfluctuation power spectrum normalization sigma_8 <= 0.8 at about the two-sigmalevel, in contrast with observations. We discuss further theoretical worknecessary to go beyond our approximations to confirm these results.Comment: 21 pages, 3 figures. References adde

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