Testing the equivalence principle in the field of the Earth: Particle physics at masses below 1 μeV?

E. G. Adelberger, C. W. Stubbs, B. R. Heckel, Y. Su, H. E. Swanson, G. Smith, J. H. Gundlach, and W. F. Rogers
Phys. Rev. D 42, 3267 – Published 15 November 1990
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Abstract

A sensitive, systematic search for feeble, macroscopic forces arising from the exchange of hypothetical ultra-low-mass bosons was made by observing the differential acceleration of two different test body pairs toward two different sources. Our differential accelerometer—a highly symmetric, continuously rotating torsion balance—incorporated several innovations that effectively suppressed systematic errors. All known sources of systematic error were demonstrated to be negligible in comparison to our fluctuating errors which are roughly 7 times larger than the fundamental limit set by the fact that we observe an oscillator at room temperature with a given damping time. Our 1σ limits on the horizontal differential acceleration of Be/Al or Be/Cu test body pairs in the field of the Earth, Δa=(2.1±2.1)×1011 cm s2 and Δa=(0.8±1.7)×1011 cm s2, respectively, set improved bounds on Yukawa interactions mediated by bosons with masses ranging between mbc23×1018 and mbc21×106 eV. For example, our constraints on infinite-range vector interactions with charges of B and of BL are roughly 10 and 2 times more sensitive than those obtained by Roll, Krotkov and Dicke using the field of the Sun. Furthermore we set stringent constraints down to λ=1 m, while those of solar experiments are weak for λ<1 AU. In terms of the weak equivalence principle in the field of the Earth, our 1σ result corresponds to mimg(Cu)mimg(Be)=(0.2±1.0)×1011. Our results also yield stringent constraints on the nonsymmetric gravitation theory of Moffat and on the anomalous acceleration of antimatter in proposed "quantum gravity" models, and have implications for lunar-ranging tests of the strong equivalence principle. Our 1σ limit on the differential acceleration of Be/Al test body pairs toward a 1.5 Mg Pb laboratory source, Δa=(0.15±1.31)×1010 cm s2, provides constraints on Yukawa interactions with ranges down to 10 cm, and on interactions whose charge is B2L.

  • Received 16 May 1990

DOI:https://doi.org/10.1103/PhysRevD.42.3267

©1990 American Physical Society

Authors & Affiliations

E. G. Adelberger, C. W. Stubbs*, B. R. Heckel, Y. Su, H. E. Swanson, G. Smith, and J. H. Gundlach

  • Physics Department, University of Washington, Seattle, Washington 98195

W. F. Rogers

  • Department of Physics and Astronomy, State University of New York at Geneseo, Geneseo, New York 14454

  • *Present address: Center for Particle Astrophysics, University of California, Berkeley, CA 94720.

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Vol. 42, Iss. 10 — 15 November 1990

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