Nirmal K. Sinha

Engineering Physics of High-Temperature Materials


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other, pile up, and form ridges, very similar to the formation of mountains and continents caused by plate tectonic forces. Ridge formations in ice may take a few seconds or minutes, but millions of years are taken to build up mountains due to plate tectonics. How can one reconcile these two apparently different phenomena? An effort for reconciliation is made in Chapters 10 and 11. As incredible as it may sound, it will be shown that an event lasting for 1 s at say 0.98 T m could be equivalent to several million years at 0.2 T m.

      Generally, materials science experimentalists and theoreticians promote the “steady‐state” aspects of deformation of materials at high temperatures. Not surprisingly, it is extended to mantle physics. Similarly, glaciologists (working only on flow of glaciers) are concerned singularly with “steady‐state” creep response. Geophysicists are certainly aware of the role of transient creep of rocks largely because of earthquake‐related problems. However, other than dislocation creep, they have largely dealt with phenomenological aspects of rheology, not necessary from the micromechanical point of view. Now, there is a growing interest among geophysicists to focus on the transient creep of geologic materials (Karato 1998; Birger 2016). However, effects of grain size on transient creep and closely related delayed elastic response of rocks at high temperatures are still to be recognized and explored.

      Geologists, geophysicists, and metallurgists do not necessarily have to deal with high‐temperature issues as much as ice engineers and glaciologists have to, simply because ice always exists at temperatures very close to its melting point. Most ice engineering problems involve extremely short‐term response well within the transient creep (Gold and Sinha 1980). Engineers dealing with ice engineering in Canada, the Northern States, Scandinavia, Russia, and China were thus baffled for a long time. No wonder, ice engineers facing complex mechanical responses of ice used to conclude, “ice is a peculiar material” – for example, its Young's modulus “depends” on grain size and changes with time and loading rates.

Schematic illustration of scanning electron micrograph of (a) a vertical section of a brine pocket at negative 30 degrees C in columnar-grained first-year sea ice with salinity of 4 percentage, and (b) details of precipitated salt crystals.

      Source: Modified from Sinha (1977).

      Even though water is the basis of life on Earth and has been the subject of the most scientific scrutiny for several centuries, the solid state of water – or ice – has rarely been considered as a “hot crystalline material.” Glaciologists may be considered as the pioneers in examining ice as a solid crystalline material for over a century, but they tend to consider glacier ice as “cold” and the subject of glaciology as special. Viscoelastic flow properties of glacier ice were formulated during the 1950s and are well known. Rarely, however, has a glacier been compared to a bed or river of molten rock or lava flowing viscoelastically (not necessarily linear viscoelastic) down the mountain side. High‐temperature creep deformation in many cases, like flow in glaciers, involves syntectonic (geology describing any process that accompanies a tectonic one) fabric development, yet this critical topic is not mentioned in the field of glaciology as an elevated temperature phenomenon. Only recently has effort been made in establishing one‐to‐one correspondence on a physical basis between the cracking and flowing characteristics in glaciers and those in semisolid lava or igneous rock undergoing complex high‐temperature flow as well.

      High‐temperature mechanical properties of materials are characterized by their creep life. Creep and fracture properties are governed by structural changes, as well as damages in the form of cavities and cracks that occur during deformation. Most tests are performed in air. It is convenient to perform tests in air, simply because providing an inert environment during tests is very difficult. However, oxidation starting from the exposed surfaces of specimens in pure metals and alloys at elevated temperatures is unavoidable. Materials are degraded or damaged by the formation of voids preferably along the grain boundaries (being at higher energy states). For example, Wilshire and Battenbough (2007) performed tensile creep and rupture tests on fine‐grained (≈40 μm) polycrystalline pure copper under truly constant stress (using the machine described in Evans and Wilshire 1985), as well as constant load at 686–823 K (about 0.5–0.6 T m), and demonstrated an increasing number of voids with increasing distance from the surface. They reported that fracture invariably occurs by cavitation, with the following observations noted: (i) Isolated grain‐boundary cavities are evident late in the primary stage during creep in both the n ∼ = 1 and n ∼ = 4.5 regimes, (ii) cavities form preferentially near specimen surfaces, with the numbers of cavities and cracks decreasing from the surface to the center due primarily to the formation of oxide particles created by oxygen ingress along grain boundaries during creep exposure (Parker and Wilshire 1980), and (iii) the incidence of cavities increases with increasing creep strain, eventually forming single‐grain‐facet cracks that are linked to producing large multigrain‐facet cracks at various locations along the gauge length of fractured specimens.

      In many respects, the above descriptions of creep cavitation and failure processes in metals (except for oxide formation) are remarkably similar to the observations of cracking activities during creep in ice (Gold 1972a, b). However, most importantly, the transparency of ice allows the use of visual and optical methods of observing the formation of cracks, as well as the use of acoustic emission methods for quantifying the kinetics of cracking activities during creep at experimental temperatures.

      The Celsius scale of temperature is almost universally accepted as the standard scale for temperature. It is based on the thermal state of pure water, which is the source for life and most abundant material on Earth's surface. In this scale, and for conditions under normal atmospheric pressure at sea level, the solidification temperature of pure water is considered as 0 °C and the boiling point is assumed to be 100 °C. Consequently, temperatures of the solid state of water (that is ice) are assigned with “negative” signs. The problem with this scale is that any temperature less than 0 °C is described as negative (−sign); a better scale is kelvin, as there is no negative temperature. However, is it a rational temperature for materials scientists to use? We will go to this question later, but let us first discuss human