Encyclopedia of Glass Science, Technology, History, and Culture. Группа авторов

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      8 8 Farges, F., Brown, G.E. Jr., Navrotsky, A. et al. (1996). Coordination chemistry of Ti(IV) in silicate glasses and melts: II. Glasses at ambient temperature and pressure. Geochim. Cosmochim. Acta 60: 3039–3053.

      9 9 Farges, F., Brown, G.E. Jr., and Rehr, J.J. (1997). Ti K‐edge XANES studies of Ti coordination and disorder in oxide compounds: comparison between theory and experiment. Phys. Rev. B 56: 1809–1819.

      10 10 Stebbins, J.F. and Xue, X. (2014). NMR spectroscopy of inorganic Earth materials. Rev. Mineral Geochem. 78: 605–653.

      11 11 McMillan, P. and Hofmeister, A.M. (1988). Infra‐red and Raman spectroscopy. Rev. Mineral Geochem. 18: 99–159.

      12 12 Kamitsos, E.I. (2014). Infrared spectroscopy of glasses. In: Modern Glass Characterisation (ed. M. Affatigato), 1–42. Hoboken, NJ: John Wiley & Sons.

      13 13 Behrens, H. and Yamashita, S. (2008). Water speciation in hydrous sodium tetrasilicate and hexasilicate melts: constraint from high temperature NIR spectroscopy. Chem. Geol. 256: 306–315.

      14 14 Behrens, H., Misiti, V., Freda, C. et al. (2009). Solubility of H2O and CO2 in ultrapotassic melts at 1200 and 1250 degrees C and pressure from 50 to 500 MPa. Am. Mineral. 94: 105–120.

      15 15 Cochain, B., Neuville, D.R., Henderson, G.S. et al. (2012). Effects of the Iron content, redox state and structure of sodium borosilicate glasses: a Raman, Mössbauer and Boron K‐edge XANES spectroscopy study. J. Am. Ceram. Soc. 94: 1–10.

      16 16 Innocenzi, P. (2003). Infrared spectroscopy of sol–gel derived silica‐based films: a spectra‐microstructure overview. J. Non Cryst. Solids 316: 309–319.

      17 17 Dubessy, J., Caumon, M.‐C., and Rull, F. (2010). Raman spectroscopy Applied to Earth Sciences and Cultural Heritage, European Mineralogical Union, vol. 12. Aberystwyth, UK: Cambrian Printers.

      18 18 Neuville, D.R., de Ligny, D., and Henderson, G.S. (2014). Advances in Raman spectroscopy applied to Earth and materials sciences. Rev. MineralGeochem. 78: 509–541.

      19 19 Richet, N.F. (2009). Heat capacity and low‐frequency vibrational density of states. Inferences for the boson peak of silica and alkali silicate glasses. Physica B 404: 3799–3806.

      20 20 Matson, D.W., Sharma, S.K., and Philpotts, J.A. (1983). The structure of high silica alkali‐silicate glasses. A Raman spectroscopic investigation. J. Non Cryst. Solids 58: 323–352.

      21 21 Speziale, S., Marquardt, H., and Duffy, T. (2014). Brillouin spectroscopy and its applications in geosciences. Rev. Mineral Geochem. 78: 543–603.

      22 22 Murakami, M. and Bass, J.D. (2010). Spectroscopic evidence for ultra‐high‐pressure polymorphism in SiO2 glass. Phys. Rev. Lett. 104: 025504.

      23 23 Johnson, J.A. and Johnson, C.E. (2005). Mössbauer spectroscopy as a probe of silicate glasses. J. Phys. Condens. Mat. 17: R318–R412.

      24 24 Nesbitt, H.W. and Bancroft, G.M. (2014). High resolution core‐ and valence‐level XPS studies of the Properties (structural, chemical and bonding) of silicate minerals and glasses. Rev. Mineral Geochem. 78: 271–329.

      25 25 Nesbitt, H.W., Bancroft, G.M., Henderson, G.S. et al. (2011). Bridging, non‐bridging and free (O2−) oxygen in Na2O‐SiO2 glasses: An X‐ray photoelectron spectroscopic (XPS) and nuclear magnetic resonance (NMR) study. J. Non Cryst. Solids 357: 170–180.

      26 26 Rossman, G.R. (2014). Optical spectroscopy. Rev. Mineral. Geochem. 78: 371–398.

      Note

      1 Reviewers:B. Mysen, Geophysical Laboratory, Carnegie Institution of Washington, Washington, DC, USAJ. F. Stebbins, Geological and Environmental Sciences, Stanford University, Stanford, CA, USA

       Christian Patzig and Thomas Höche

       Fraunhofer Institute for Microstructure of Materials and Systems IMWS, Halle (Saale), Germany

      A homogeneous glass by definition lacks a microstructure at a scale larger than a few nanometers. As soon as actual inhomogeneities occur, in contrast, a detailed picture of their size, distribution, composition, and spatial arrangement becomes important to understand the properties of the material. In turn, the improved capabilities of microstructural studies in terms of spatial and elemental resolution are becoming increasingly important to optimize crystallization or phase separation and to achieve the desired microstructure and associated properties (Chapter 7.11). As a matter of fact, the beauty and challenge of glasses and glass ceramics is their diversity and complexity.

      The purpose of this chapter thus is to review the main microstructural methods commonly used to study inhomogeneous glass‐based materials. In preamble, however, it is important to note that studying extremely small volumes in great detail can result in “knowing everything about nothing.” In other words, it is critically important to make sure that the information gathered locally is actually representative for larger volumes. To achieve this goal, highly resolved information must be combined with additional integral measurements to get a broad picture. In addition, artifacts introduced upon either preparation or investigation of the sample must be avoided. And one should also be extremely careful with in situ microstructural experiments where, because of dramatic differences in the surface‐to‐volume ratio, annealing can easily lead to results not observed in the bulk. For this reason, one is advised to freeze a microstructure evolution by stopping it at specific steps and to use multiple samples taken from different stages for gaining a “full‐picture” characterization.

      When dealing with the early stages of crystallization or nanoscale phase separation, it is obvious that light microscopy is not an appropriate analysis technique because its optical resolution of a few 100 nm, which is limited by the wavelengths of visible light, is two orders of magnitude too low. Fortunately, however, there are various ways to improve spatial resolution. As described in Chapter 2.2, the first is to probe the material with photons of shorter wavelengths such as X‐rays: at 154 pm, the wavelength of Cu‐Kα X‐rays is for instance 1000 times shorter than that of visible light. A second way is to take advantage of the wave‐particle dualism of electrons or ions. Under accelerating voltages of 25 and 200 kV, the electron wavelengths are even shorter than that of typical X‐rays, with values of 8 and 2.5 pm, respectively. As a matter of fact, the former value is typical for studies of sample surfaces by scanning electron microscopy (SEM), whereas the latter applies to investigations by transmission electron microscopy (TEM) of bulk samples with a thickness of a few tens of nanometers at most, to limit electron absorption. In addition to these two techniques, to which we will pay particular attention, the third way to achieve high resolution will also be described. It relies on the use of scanning probes whereby a needle that is atomically sharp at its end is moved over the sample surface by a piezo drive that must be highly precise, since the key to resolution is, in this case, the accuracy of the needle position.

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