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ASTROPHYSICS. Atom-interferometry constraints on dark energy

P Hamilton¹, M Jaffe¹, P Haslinger¹

¹Department of Physics, 366 Le Conte Hall MS 7300, University of California-Berkeley, Berkeley, CA 94720, USA.

Science (New York, N.Y.)

|August 22, 2015

Abstract:

If dark energy, which drives the accelerated expansion of the universe, consists of a light scalar field, it might be detectable as a "fifth force" between normal-matter objects, in potential conflict with precision tests of gravity. Chameleon fields and other theories with screening mechanisms, however, can evade these tests by suppressing the forces in regions of high density, such as the laboratory. Using a cesium matter-wave interferometer near a spherical mass in an ultrahigh-vacuum chamber, we reduced the screening mechanism by probing the field with individual atoms rather than with bulk matter. We thereby constrained a wide class of dark energy theories, including a range of chameleon and other theories that reproduce the observed cosmic acceleration.

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