Multiloop atom interferometer measurements of chameleon dark energy in microgravity

Sheng-wey Chiow and Nan Yu
Phys. Rev. D 97, 044043 – Published 28 February 2018

Abstract

Chameleon field is one of the promising candidates of dark energy scalar fields. As in all viable candidate field theories, a screening mechanism is implemented to be consistent with all existing tests of general relativity. The screening effect in the chameleon theory manifests its influence limited only to the thin outer layer of a bulk object, thus producing extra forces orders of magnitude weaker than that of the gravitational force of the bulk. For pointlike particles such as atoms, the depth of screening is larger than the size of the particle, such that the screening mechanism is ineffective and the chameleon force is fully expressed on the atomic test particles. Extra force measurements using atom interferometry are thus much more sensitive than bulk mass based measurements, and indeed have placed the most stringent constraints on the parameters characterizing chameleon field. In this paper, we present a conceptual measurement approach for chameleon force detection using atom interferometry in microgravity, in which multiloop atom interferometers exploit specially designed periodic modulation of chameleon fields. We show that major systematics of the dark energy force measurements, i.e., effects of gravitational forces and their gradients, can be suppressed below all hypothetical chameleon signals in the parameter space of interest.

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  • Received 16 August 2017

DOI:https://doi.org/10.1103/PhysRevD.97.044043

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsAtomic, Molecular & Optical

Authors & Affiliations

Sheng-wey Chiow and Nan Yu*

  • Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA

  • *nan.yu@jpl.nasa.gov

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Issue

Vol. 97, Iss. 4 — 15 February 2018

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