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1 Department of Earth and Planetary Science, Washington University, St. Louis, Missouri 63130, U.S.A.
2 Department of Physics and Pre-engineering, Delaware State University, Dover, Delaware 19901, U.S.A.
Correspondence: * E-mail: hofmeist{at}levee.wustl.edu
Infrared reflectance, thin-film absorbance, and polarized Raman spectra were acquired from ~100 to ~4000 cm1 from polycrystalline garnets along the pyrope (Py = Mg3Al2Si3O12)-majorite [Mj = Mg3(MgSi)Si3O12 ] join. We measured Py100, Mj39, Mj45, Mj80, and natural single-crystal, nearly end-member pyrope. Consistency is obtained between measured absorption spectra and absorption coefficients calculated through Kramers-Kronig analysis of reflectivity (R) data, if R-values are scaled to account for losses through scattering. The widths of the lattice modes double from each end-member toward the middle of the binary, whereas frequencies are nearly independent of composition. Strong polarization of Raman peaks of all our samples except pyrope shows that the space group is reduced from cubic, even for the Al-rich majorites. The largest number of IR or Raman peaks is observed for Mj80. The number of peaks for Al-rich majorites lies between those seen for cubic pyrope and I41/a majorite. The behavior of symmetry-breaking modes supports the I41/acd space group, which was inferred from X-ray data for Mj contents near 30 to 45% (Nakatsuka et al. 1999a). Also, the internal mode types that are expected for isolated SiO4 tetrahedra in any garnet-like structure do not fully describe the patterns of peaks seen for some intermediate compositions along the Py-Mj join. The appearance of Sioct-O-Sitet bending modes in the available spectral data for Mj contents near 3040 and 8090%, but not near 4550%, is attributed to two-mode behavior. Specifically, disruption of the structural chain -Sioct-O-Sitet-O-Sioct-O-Sitet-in Si-rich majorites by units such as

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