Diluting the cosmological constant in infinite volume extra dimensions

By G. Dvali, G. Gabadadze, M. Shifman. 2002

178 citations recorded by the source corpus.

We argue that the cosmological constant problem can be solved in a braneworld model with infinite-volume extra dimensions, avoiding no-go arguments applicable to theories that are four-dimensional in the infrared. Gravity on the brane becomes higher-dimensional at super-Hubble distances, which entails that the relation between the acceleration rate and vacuum energy density flips upside down compared to the conventional one. The acceleration rate decreases with increasing the energy density. The experimentally acceptable rate is obtained for the energy density larger than (1 TeV)$^4$. The results are stable under quantum corrections because supersymmetry is broken only on the brane and stays exact in the bulk of infinite volume extra space. Consistency of 4D gravity and cosmology on the brane requires the quantum gravity scale to be around $10^{-3}$ eV. Testable predictions emerging within this approach are: (i) simultaneous modifications of gravity at sub-millimeter and the Hubble scales; (ii) Hagedorn-type saturation in TeV energy collisions due to the Regge spectrum with the spacing equal to $10^{-3}$ eV.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/7994f03fa87b1920cdf19392e2fa8073f5cdeb66

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In Astronomy and Astrophysics

  1. Lavinia Heisenberg
  2. Claudia de Rham
  3. A. Filippenko
  4. R. Kirshner
  5. Weidong Li
  6. A. Riess
  7. Tsutomu Kobayashi
  8. M. Zumalacárregui

In Nuclear and High Energy Physics

  1. Claudia de Rham
  2. Lavinia Heisenberg
  3. A. Tolley
  4. Kurt Hinterbichler
  5. Tsutomu Kobayashi
  6. K. Koyama
  7. J. Khoury
  8. Alberto Nicolis

In Statistical and Nonlinear Physics

  1. Claudia de Rham
  2. Lavinia Heisenberg
  3. Alberto Nicolis
  4. E. Trincherini
  5. J. Khoury
  6. A. Tolley
  7. R. Rattazzi
  8. N. Arkani-Hamed

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