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PhysRevLett.129.131302.pdf
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Final Published Version
Affiliation
Wyant College of Optical Sciences, University of ArizonaIssue Date
2022
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American Physical SocietyCitation
Betz, J., Manley, J., Wright, E. M., Grin, D., & Singh, S. (2022). Searching for Chameleon Dark Energy with Mechanical Systems. Physical Review Letters, 129(13).Journal
Physical Review LettersRights
Copyright © 2022 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.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. © 2022 American Physical Society.Note
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0031-9007Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1103/PhysRevLett.129.131302