Chameleon cosmology

Justin Khoury and Amanda Weltman
Phys. Rev. D 69, 044026 – Published 27 February 2004
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Abstract

The evidence for the accelerated expansion of the Universe and the time dependence of the fine-structure constant suggests the existence of at least one scalar field with a mass of order H0. If such a field exists, then it is generally assumed that its coupling to matter must be tuned to unnaturally small values in order to satisfy the tests of the equivalence principle (EP). In this paper, we present an alternative explanation which allows scalar fields to evolve cosmologically while having couplings to matter of order unity. In our scenario, the mass of the fields depends on the local matter density: the interaction range is typically of order 1 mm on Earth (where the density is high) and of order 10104AU in the solar system (where the density is low). All current bounds from tests of general relativity are satisfied. Nevertheless, we predict that near-future experiments that will test gravity in space will measure an effective Newton’s constant different by order unity from that on Earth, as well as EP violations stronger than currently allowed by laboratory experiments. Such outcomes would constitute a smoking gun for our scenario.

  • Received 15 September 2003

DOI:https://doi.org/10.1103/PhysRevD.69.044026

©2004 American Physical Society

Authors & Affiliations

Justin Khoury and Amanda Weltman

  • Institute for Strings, Cosmology and Astroparticle Physics, Columbia University, New York, New York 10027, USA

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Issue

Vol. 69, Iss. 4 — 15 February 2004

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