Accuracy estimation of the O216+ transition frequencies targeting the search for the variation in the proton-electron mass ratio

Masatoshi Kajita
Phys. Rev. A 95, 023418 – Published 22 February 2017

Abstract

We estimate the Stark and Zeeman shifts in the transition frequencies of the O216+ molecular ion as a step in the search for the variation in the proton-to-electron mass ratio μ. The X2Πv=21a4Πv=0 or the X2Πv=21a4Πv=1 transition frequencies (THz region) of the O216+ molecular ion have particularly high sensitivity to the variation in μ. Note also that the Stark shift in the O216+ transition frequencies is expected to be much smaller than that for heteronuclear diatomic molecules. However, the actual systematic uncertainties for the O216+ transition frequencies have never been estimated. We estimated the Stark and Zeeman shifts in the different O216+ transition frequencies. When the molecular ions in a string crystal formed in a linear trap (trap electric field <0.1 V/cm, and Stark shift <1020) are used, the X2Π1/2(v,J)=(0,1/2)(v,1/2)(v1) transition frequencies are most advantageous for the search for the variation in μΔμ/μ<1017 because the Zeeman shift is easily suppressed to lower than 1018 and the electric quadrupole shift is zero. On the other hand, the X2Π1/2v,J=21,1/2a4Π1/2v,J=0,1/2 transition frequency has another merit in that the positive Stark shift induced by the trap electric field can be canceled by the quadratic Doppler shift. Therefore, the measurement using molecular ions in a Coulomb crystal broadened in the radial direction is also possible, when the Zeeman shift is effectively eliminated.

  • Received 14 November 2016

DOI:https://doi.org/10.1103/PhysRevA.95.023418

©2017 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & Optical

Authors & Affiliations

Masatoshi Kajita*

  • National Institute of Information and Communications Technology, Koganei, Tokyo 184-8795, Japan

  • *kajita@nict.go.jp; http://www.nict.go.jp/en/index.html

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Issue

Vol. 95, Iss. 2 — February 2017

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