Searching for Chameleon Dark Energy with Mechanical Systems

J. Betz, J. Manley, E. M. Wright, D. Grin, and S. Singh
Phys. Rev. Lett. 129, 131302 – Published 23 September 2022
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Abstract

A light scalar field framework of dark energy, sometimes referred to as quintessence, introduces a fifth force between normal matter objects. Screening mechanisms, such as the chameleon model, allow the scalar field to be almost massless on cosmological scales while simultaneously evading laboratory constraints. We explore the ability of existing mechanical systems to directly detect the fifth force associated with chameleons in an astrophysically viable regime where it could be dark energy. We provide analytical expressions for the weakest accessible chameleon model parameters in terms of experimentally tunable variables and apply our analysis to two mechanical systems: levitated microspheres and torsion balances, showing that the current generation of these experiments have the sensitivity to rule out a significant portion of the proposed chameleon parameter space. We also indicate regions of theoretically well-motivated chameleon parameter space to guide future experimental work.

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  • Received 10 February 2022
  • Revised 20 July 2022
  • Accepted 29 August 2022

DOI:https://doi.org/10.1103/PhysRevLett.129.131302

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsInterdisciplinary PhysicsParticles & FieldsAtomic, Molecular & Optical

Authors & Affiliations

J. Betz1, J. Manley2, E. M. Wright3, D. Grin4, and S. Singh2,1,*

  • 1Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA
  • 2Department of Electrical and Computer Engineering, University of Delaware, Newark, Delaware 19716, USA
  • 3Wyant College of Optical Sciences, University of Arizona, Tucson, Arizona 85721, USA
  • 4Department of Physics and Astronomy, Haverford College, Haverford, Pennsylvania 19041, USA

  • *swatis@udel.edu

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Issue

Vol. 129, Iss. 13 — 23 September 2022

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