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Plasma versus Drude Modeling of the Casimir Force: Beyond the Proximity Force Approximation

Michael Hartmann, Gert-Ludwig Ingold, and Paulo A. Maia Neto
Phys. Rev. Lett. 119, 043901 – Published 24 July 2017

Abstract

We calculate the Casimir force and its gradient between a spherical and a planar gold surface. Significant numerical improvements allow us to extend the range of accessible parameters into the experimental regime. We compare our numerically exact results with those obtained within the proximity force approximation (PFA) employed in the analysis of all Casimir force experiments reported in the literature so far. Special attention is paid to the difference between the Drude model and the dissipationless plasma model at zero frequency. It is found that the correction to PFA is too small to explain the discrepancy between the experimental data and the PFA result based on the Drude model. However, it turns out that for the plasma model, the corrections to PFA lie well outside the experimental bound obtained by probing the variation of the force gradient with the sphere radius [D. E. Krause et al., Phys. Rev. Lett. 98, 050403 (2007)]. The corresponding corrections based on the Drude model are significantly smaller but still in violation of the experimental bound for small distances between plane and sphere.

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  • Received 11 May 2017

DOI:https://doi.org/10.1103/PhysRevLett.119.043901

© 2017 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
General Physics

Authors & Affiliations

Michael Hartmann1, Gert-Ludwig Ingold1, and Paulo A. Maia Neto2

  • 1Universität Augsburg, Institut für Physik, 86135 Augsburg, Germany
  • 2Instituto de Física, Universidade Federal do Rio de Janeiro, CP 68528, Rio de Janeiro, Rio de Janeiro 21941-909, Brazil

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Issue

Vol. 119, Iss. 4 — 28 July 2017

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