Constraints on non-Newtonian gravity and light elementary particles from measurements of the Casimir force by means of a dynamic atomic force microscope

G. L. Klimchitskaya, U. Mohideen, and V. M. Mostepanenko
Phys. Rev. D 86, 065025 – Published 19 September 2012

Abstract

We derive constraints on corrections to Newtonian gravity of the Yukawa type and light elementary particles from two recently performed measurements of the gradient of the Casimir force. In the first measurement the configuration of two Au surfaces has been used, whereas in the second a nonmagnetic metal Au interacted with a magnetic metal Ni. In these configurations one arrives at different and similar, respectively, theoretical predictions for the Casimir force when the competing theoretical approaches are employed. Nevertheless, we demonstrate that the constraints following from both experiments are in mutual agreement and in line with constraints obtained from earlier measurements. This confirms the reliability of constraints on non-Newtonian gravity obtained from measurements of the Casimir force.

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  • Received 30 June 2012

DOI:https://doi.org/10.1103/PhysRevD.86.065025

© 2012 American Physical Society

Authors & Affiliations

G. L. Klimchitskaya1, U. Mohideen2, and V. M. Mostepanenko1

  • 1Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences, St. Petersburg 196140, Russia and Institute for Theoretical Physics, Leipzig University, Postfach 100920, D-04009 Leipzig, Germany
  • 2Department of Physics and Astronomy, University of California, Riverside, California 92521, USA

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Issue

Vol. 86, Iss. 6 — 15 September 2012

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