Abstract
Abstract
We derive the best possible bounds that can be placed on Yukawa-- and chameleon--like modifications to the Newtonian gravitational potential with a cavity optomechanical quantum sensor. By modelling the effects on an oscillating source-sphere on the optomechanical system from first-principles, we derive the fundamental sensitivity with which these modifications can be detected in the absence of environmental noise. In particular, we take into account the large size of the optomechanical probe compared with the range of the fifth forces that we wish to probe and quantify the resulting screening effect when both the source and probe are spherical. Our results show that optomechanical systems in high vacuum could, in principle, further constrain the parameters of chameleon-like modifications to Newtonian gravity.
Funder
Engineering and Physical Sciences Research Council
Knut och Alice Wallenbergs Stiftelse
Alexander von Humboldt-Stiftung
H2020 Marie Skłodowska-Curie Actions
FP7 Ideas: European Research Council
Royal Society
Subject
General Physics and Astronomy
Cited by
8 articles.
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