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Degravitation of the cosmological constant and graviton width

Gia Dvali, Stefan Hofmann, and Justin Khoury
Phys. Rev. D 76, 084006 – Published 9 October 2007

Abstract

We study the possibility of decoupling gravity from the vacuum energy. This is effectively equivalent to promoting Newton’s constant to a high-pass filter that degravitates sources of characteristic wavelength larger than a certain macroscopic (super) horizon scale L. We study the underlying physics and the consistency of this phenomenon. In particular, the absence of ghosts, already at the linear level, implies that in any such theory the graviton should either have a mass 1/L, or be a resonance of similar width. This has profound physical implications for the degravitation idea.

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  • Received 25 March 2007

DOI:https://doi.org/10.1103/PhysRevD.76.084006

©2007 American Physical Society

Authors & Affiliations

Gia Dvali1, Stefan Hofmann2, and Justin Khoury2

  • 1Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003, USA
  • 2Perimeter Institute for Theoretical Physics, 31 Caroline St. N., Waterloo, ON, N2L 2Y5, Canada

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Issue

Vol. 76, Iss. 8 — 15 October 2007

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Images

  • Figure 1
    Figure 1
    The weak coupling (r>r) and strong coupling (r<r) solution of (56) for the Stückelberg field in the case of a point charge at r=0. The change in the behavior at r is analogous to the gravity case.Reuse & Permissions
  • Figure 2
    Figure 2
    The effective potential for the metric function f(t), as given by (99).Reuse & Permissions
  • Figure 3
    Figure 3
    Conventions for the branch cut in the integrand for I. This function has two poles, at ω+ and ω, which lie in the upper and lower half-plane, respectively. The pole in the lower half-plane, however, lies on the second Riemann sheet and can be accessed by going under the branch cut.Reuse & Permissions
  • Figure 4
    Figure 4
    Choice of contour for I(t>0).Reuse & Permissions
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