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==Effects of time and temperature== [[Image:DiagrammeTTT.GIF|thumb|Time-temperature transformation (TTT) diagram for steel. The red curves represent different cooling rates (velocity) when cooled from the upper critical (A3) temperature. V1 (quenching) produces martensite. V2 (normalizing) produces both pearlite and martensite, V3 (annealing) produces bainite mixed with pearlite.|400x400px]] Proper heat treating requires precise control over temperature, time held at a certain temperature and cooling rate.<ref>{{Cite book |title=Heat Treatment: Principles and Techniques |first1=T. V. |last1=Rajan |first2=C. P. |last2=Sharma |first3=Ashok |last3=Sharma |publisher=Prentence Hall |year=1992 |ref={{harvid|Rajan|Sharma|1992}} |page=1 }}</ref> With the exception of stress-relieving, tempering, and aging, most heat treatments begin by heating an alloy beyond a certain transformation, or arrest (A), temperature. This temperature is referred to as an "arrest" because at the A temperature the metal experiences a period of [[hysteresis]]. At this point, all of the heat energy is used to cause the crystal change, so the temperature stops rising for a short time (arrests) and then continues climbing once the change is complete.<ref>''New Edge of the Anvil: A Resource Book for the Blacksmith'' by Jack Andrews --Shipjack Press 1994 Page 93--96</ref> Therefore, the alloy must be heated above the critical temperature for a transformation to occur. The alloy will usually be held at this temperature long enough for the heat to completely penetrate the alloy, thereby bringing it into a complete solid solution. Iron, for example, has four critical-temperatures, depending on carbon content. Pure iron in its alpha (room temperature) state changes to nonmagnetic gamma-iron at its A<sub>2</sub> temperature, and [[Welding|weldable]] delta-iron at its A<sub>4</sub> temperature. However, as carbon is added, becoming steel, the A<sub>2</sub> temperature splits into the A<sub>3</sub> temperature, also called the [[austenizing]] temperature (all phases become austenite, a solution of gamma iron and carbon) and its A<sub>1</sub> temperature (austenite changes into pearlite upon cooling). Between these upper and lower temperatures the pro eutectoid phase forms upon cooling. Because a smaller grain size usually enhances mechanical properties, such as [[toughness]], [[shear strength]] and [[tensile strength]], these metals are often heated to a temperature that is just above the upper critical temperature, in order to prevent the grains of solution from growing too large. For instance, when steel is heated above the upper critical-temperature, small grains of austenite form. These grow larger as the temperature is increased. When cooled very quickly, during a martensite transformation, the austenite grain-size directly affects the martensitic grain-size. Larger grains have large grain-boundaries, which serve as weak spots in the structure. The grain size is usually controlled to reduce the probability of breakage.<ref>{{harvnb|Rajan|Sharma|1992|pages=62β67}}</ref> The diffusion transformation is very time-dependent. Cooling a metal will usually suppress the precipitation to a much lower temperature. Austenite, for example, usually only exists above the upper critical temperature. However, if the austenite is cooled quickly enough, the transformation may be suppressed for hundreds of degrees below the lower critical temperature. Such austenite is highly unstable and, if given enough time, will precipitate into various microstructures of ferrite and cementite. The cooling rate can be used to control the rate of grain growth or can even be used to produce partially martensitic microstructures.<ref>{{harvnb|Dossett|Boyer|2006|pages=23β25}}</ref> However, the martensite transformation is time-independent. If the alloy is cooled to the martensite transformation (M<sub>s</sub>) temperature before other microstructures can fully form, the transformation will usually occur at just under the speed of sound.<ref>''The physics of phase transitions: concepts and applications'' By Pierre Papon, Jacques Leblond, Paul Herman Ernst Meijer - Springer-Verlag Berlin Heidelberg 2006 Page 66</ref> When austenite is cooled but kept above the martensite start temperature Ms so that a martensite transformation does not occur, the austenite grain size will have an effect on the rate of nucleation, but it is generally temperature and the rate of cooling that controls the grain size and microstructure. When austenite is cooled extremely slowly, it will form large ferrite crystals filled with spherical inclusions of cementite. This microstructure is referred to as "sphereoidite". If cooled a little faster, then coarse pearlite will form. Even faster, and fine pearlite will form. If cooled even faster, [[bainite]] will form, with more complete bainite transformation occurring depending on the time held above martensite start Ms. Similarly, these microstructures will also form, if cooled to a specific temperature and then held there for a certain time.<ref>{{harvnb|Rajan|Sharma|1992}}</ref> Most non-ferrous alloys are also heated in order to form a solution. Most often, these are then cooled very quickly to produce a martensite transformation, putting the solution into a [[supersaturation|supersaturated]] state. The alloy, being in a much softer state, may then be [[cold forming|cold worked]]. This causes [[work hardening]] that increases the strength and hardness of the alloy. Moreover, the defects caused by [[plastic deformation]] tend to speed up precipitation, increasing the hardness beyond what is normal for the alloy. Even if not cold worked, the solutes in these alloys will usually precipitate, although the process may take much longer. Sometimes these metals are then heated to a temperature that is below the lower critical (A<sub>1</sub>) temperature, preventing recrystallization, in order to speed-up the precipitation.<ref>{{harvnb|Dossett|Boyer|2006|page=231}}</ref><ref>{{harvnb|Rajan|Sharma|1992|pages=187β190, 321}}</ref><ref>''Manufacturing technology: foundry, forming and welding'' By Rao - Tata McGraw-Hill 1998 Page 55</ref>
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