Gradient of the Casimir force between Au surfaces of a sphere and a plate measured using an atomic force microscope in a frequency-shift technique

C.-C. Chang, A. A. Banishev, R. Castillo-Garza, G. L. Klimchitskaya, V. M. Mostepanenko, and U. Mohideen
Phys. Rev. B 85, 165443 – Published 25 April 2012

Abstract

We present measurement results for the gradient of the Casimir force between an Au-coated sphere and an Au-coated plate obtained by means of an atomic force microscope operated in a frequency-shift technique. This experiment was performed at a pressure of 3×108 Torr with a hollow glass sphere of 41.3 μm radius. Special attention is paid to electrostatic calibrations, including the problem of electrostatic patches. All calibration parameters are shown to be separation independent after the corrections for mechanical drift are included. The gradient of the Casimir force was measured in two ways with applied compensating voltage to the plate and with different applied voltages and subsequent subtraction of electric forces. The obtained mean gradients are shown to be in mutual agreement and in agreement with previous experiments performed using a micromachined oscillator. The obtained data are compared with theoretical predictions of the Lifshitz theory including corrections beyond the proximity force approximation. An independent comparison with no fitting parameters demonstrated that the Drude model approach is excluded by the data at a 67% confidence level over the separation region from 235 to 420 nm. The theoretical approach using the generalized plasmalike model is shown to be consistent with the data over the entire measurement range. Corrections due to the nonlinearity of oscillator are calculated and the application region of the linear regime is determined. A conclusion is made that the results of several performed experiments call for a thorough analysis of the basics of the theory of dispersion forces.

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  • Received 24 January 2012

DOI:https://doi.org/10.1103/PhysRevB.85.165443

©2012 American Physical Society

Authors & Affiliations

C.-C. Chang1, A. A. Banishev1, R. Castillo-Garza1, G. L. Klimchitskaya2, V. M. Mostepanenko3, and U. Mohideen1

  • 1Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
  • 2North-West Open Technical University, St. Petersburg, 195597, Russia
  • 3Central Astronomical Observatory of the Russian Academy of Sciences, St. Petersburg, 196140, Russia

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Vol. 85, Iss. 16 — 15 April 2012

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