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We performed the measurements on the U2B IR beam line at the National Synchrotron Light Source (NSLS), using a Fourier Iransform-IR (Nicolel 750) spectrometer with KBr beam splitter. The characteristics of the beam line are given by G. L. Carr et al. [Rev. Sci. Instrum. 66, 1643 (1995)]. Synchrotron light passes through the spectrometer and is focused into the diamond anvil cell to spots 20 to 30 μm in diameter (in the visible), using a custom-built IR microscope with Cassegrain mirror objective (numerical aperture = 0.25, ×8). For absorption measurements, a ZnSe lens placed inside a Mao-Bell diamond-anvil cell collects the light transmitted through the sample and images it on a mercury-cadmium telluride detector (MCT). Reflected light is collected by the same mirror objective, which illuminates the sample, applying a half-mirror beam splitter. A separate MCT detector was used to record the reflectivity, which permitted collection of complementary absorption and reflectivity spectra at each pressure.
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9444238161
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in preparation
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V. V. Struzhkin, A. F. Goncharov, M. Somayazulu, R. J. Hemley, H. K. Mao, in preparation.
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9444260601
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note
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1 as a Fano-type interference between a narrow band and the continuum. We find, however, that the observed line shape does not necessarily require interference, because two independent oscillators (the first, a relatively weak and narrow IR band inside a second, the strong and broad reststrahlen band) also give rise to a Fano-like absorption as a result of the complex behavior of the optical conslants (27).
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note
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Alternatively, calculations using a double-well potential model for the hydrogen bond suggest that this could also arise from splitting of energy levels associated with the changing barrier height (21).
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30
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9444228469
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note
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The double-well potential calculations also predict a change in proton motion at these pressures (21). Although the spectroscopic features at 150 to 160 GPa are indicative of a type of Fermi resonance, a second phase transition cannot be ruled out
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32
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9444282274
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note
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We are grateful to P Loubeyre, Ph. Pruzan, and J.-M. Besson for comments on the manuscript. This work was supported by the National Science Foundation and NASA. The NSLS is supported by the Department of Energy under contract DE-AC02-76-CH00016.
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