8.2.3 It's a Long way to Nirvana
|The Aluminum - Copper Experiment|
|Let's look at a classical example that uses our strategies in a particularly transparent way. Thanks go to Michael Ashby, David Jones and their grad students who most likely did the actual work.|
|The idea was to harden Aluminum (Al) by adding a small
amount of copper (Cu). This is important for making superior beer cans (and the cans for less interesting beverages).
You don't want to entrust your beer to any can, you want a can with properties
that are "just
right". Here is a short list:
|One of many possible ways to go is to use copper (Cu) as an alloying element. It must do the job already in small quantities since copper is expensive. In the "Ashby and Jones" an extensive systematic study is reported about what you can do with copper in aluminum. It serves as a paradigm, a model case for hardening metals by the mechanisms of|
|I will guide you through this study because what is happening in the Al-Cu system is typical for most alloysbut far easier to understand than what happens in the Fe-C-some dirt system. Note that what follows is not the way the materials for real beer cans are made, it just provides basic and systematic knowledge for that venture.|
|First we alloy very pure aluminum (Al) with about 4 % of copper (Cu) and hold it at around 550 oC (932 oF) for a while. In other words: we make a rather ideal and expensive binary system.|
|Nothing helps, you now need to
look a the aluminum (Al) -
copper (Cu) phase diagram. Use the link.
Yes, it is horribly complex; a real nightmare. But if we just look at the aluminum-rich part, it is actually simple. Here goes:
|In the Al-rich part, with just 4 % copper (Cu),
at 550 oC (932 oF) we
just have Cu dissolved in aluminum or the
usual a-phase. That means that single Cu atoms are
occupying the sites of Al atoms in its fcc lattice. The copper atoms thus are
impurity atoms of the substitutional kind. You just as well could call then
doping atoms because they are intentionally
introduced, but nobody does that. This term is more or less reserved for
properties by introducing impurities. We do call them "alloying element", though.
Our starting material at 550 oC thus is poly-crystalline aluminum with 4 % of copper (Cu) atoms fully dissolved, some dislocations and vacancies, and not much else.
At lower temperatures the crystal obviously needs to produce a few large CuAl2 precipitates for achieving nirvana. The chemical compound CuAl2 is also called the theta (Q) phase
quench to room temperature.
You do that so fast that no precipitation occurs during the cooling. In the
laboratory we can do that, effectively "freezing in" the high
Then you temper by going up to a constant 150 oC (302 oF), i.e. you employ strategy No. 1.
|When you start at the 150 oC, you now have exactly what you had at 550 oC: 4% copper atomically dissolved in an aluminium polycrystal. The only difference is that at 150 oC the crystal is unhappy about that. Very unhappy. It will now do whatever it can to remedy the situation and to establish the proper nirvana state, which is almost copper-free aluminum plus CuAl2 precipitates. You also can call it a mixture of the a and Q phase; same thing.|
|So all you do next is to let your specimen sit at the chosen temperature for a while (employing strategy No. 3). You picked 150 oC because at room temperature your aluminum cannot do much during your life time; everything is pretty much immobilized. If you temper at 150 oC, there is enough thermal energy to allow precipitation to happen, just rather s-l-o-w-l-y because the Cu atoms move rather sluggishly at that temperature.|
|That is good because it gives us enough time to observe at our leisure what is going on.|
|The important point is that the driving force for precipitation is large at this low temperature because the crystal can gain a lot of energy by getting rid of surplus copper atoms.|
| A temperature of 150 oC
combines an overwhelming need for making precipitates with some sluggishness in
doing things. We're thus heeding the "golden rule"
from before and control nucleation and kinetics. The crystal has no choice but
to start a lot of very small precipitates all over the place.
If there is a sufficient number of defects around, nucleation will now start at those defects, i.e. we have heterogeneous nucleation. Otherwise nucleation will be homogeneous but the details don't matter for our purpose here. We just will produce a large number of nuclei soon after we reached the final 150 oC, and we do not need to care exactly how that happens and exactly how large that number will be.
|Before I go on let's reconsider the concept of the driving force; it is really important (you might want to go to the bathroom now if you remember the preceding chapter).|
driving force for things to
happen is just a measure of how much the crystal has to gain (in terms of
energy) by doing something that gets it closer to nirvana.
Consider steel just a few centigrade below the austenite-pearlite transition temperature. Yes, turning into pearlite would be better than remaining austenite, but just a little bit. You, the crystal, will go for it but not with real zest and vigor. The driving force for the transition is small. It may happen rather quickly anyway because everything is very mobile.
Now consider that you quenched the steel very quickly to several 100 centigrades below the transition temperature. The crystal wants the same structure as in the case above but turning to pearlite at this temperature would be far better than being austenite, and transformation becomes supremely important. The driving force for the transition is large.
The ominous "driving force" invoked a few times already thus simply measures the reduction of the distance to nirvana (the gain in energy in science speak) that the crystal can realize under the circumstances. Needless to say, we can calculate that and express it in a cold hard number.
The message is clear:
|Crystals are like humans in this
respect, with the exception that they are always reasonable. Humans, just like crystals, are
less inclined to do the right thing under circumstances where the benefit is
small. For example, stopping overspending and being thrifty becomes a far more
urgent business when your debtors are closing in with swords drawn.
As I'm writing this (July 31st 2011) bankruptcy for the USA is just two days away and politicians become frantic. Greece, very close to bankruptcy for about a year by now, is extremely agitated and induces desperate measures: frequent meetings of European heads of states, transfer of more than hundred billons of Euros (> 1010 ) that do not really exist, and severe violations of about every European treaty.
Two years ago, the situation was not all that different but the political driving forces were much smaller because the rating agencies had not yet drawn their swords. However, in contrast to the forces driving crystals, we cannot calculate political driving forces precisely, because large amounts of irrationality and stupidity are involved that do not surrender to (mathematical) reason.
|Like always, there is a catch to producing a high density of small precipitates via large driving forces, meaning large degrees of sudden undercooling by quenching. While this will produce the nuclei for many very small precipitates, at low temperatures things move slowly. Those nuclei will take forever to grow to the size you want. Growth means that Cu atoms move by diffusion from the depth of the Al crystal to the nuclei.. If they diffuse slowly, growth will be sluggish.|
|What can you do about this? Well,
here we don't want to do anything about it because we like whatever happens to
happen slowly. If we would want many nuclei but not-so-sluggish growth, we
employ some smarter temperature
profiling: Quench to a low temperature that produces a large driving
force and thus produces a lot of nuclei. After enough time has elapsed to form
many tiny nuclei, you go up to a specified higher temperature. Growth now is
brisk but some of the smaller precipitates will dissolve and some others may
get too large because Ostwald ripening cannot be avoided.
If needs be, repeat the process, perhaps with some in-between steps.
That's exactly what we do with silicon if we want to grow many silicon dioxide precipitates, which we may like to have in certain parts of the crystal.
|Does this sound a bit like working with wootz steel? Yes, indeed - all reports agree that the smith was employing many temperature cycles.|
|Except, he did it in order to obtain just a
few large precipitates, the exact opposite
of what I described just above. He needs to do this so he can produce the
famous "water" structure in this high-carbon or hypereutectoid steel.
We'll come to that later in more detail.
Here you just can take it as hint that the golden rule is rather powerful, indeed, provided you know what you are doing. If you don't know what you are doing, you need to have a recipe, based on centuries of experience and untold failures, that works at least occasionally. "Untold failures" means exactly that: we have never heard, read or found the results of forging attempts that failed to produce a superior wootz blade!
|Back to our Aluminum-copper alloy. After tempering for some specified time at 150 oC (302 oF), you stop whatever is going on by now quenching to room temperature (strategy 1), where not much happens anymore. Then you test your tempered Al(4%Cu) alloy for tensile strength or hardness. That gives you just one data point for the curve in the figure below. Next you analyze your specimen by everything you have (metallography, electron microscopy, ...) to ascertain exactly what kind of structure was produced.|
|Then you repeat the experiment with
a new sample, waiting a little longer at 150 oC (302 oF)
before you do the tensile test and the structure analysis.
Then you repeat the experiment....
|When you're done, you get the curve shown below.|
|Then you repeat the whole set of experiments but with specimen where only 3 % Cu was used for alloying.|
| This gives another curve for this
Then you repeat the whole set of experiments with 5 % Cu, and so on.
When you're done, you repeat everything once more but now you hold the samples at 170 oC, or 140 oC.
|And so on at (almost) infinitum.|
|A high and mighty director of a large research establishment once put it like that: "After doing this kind of work for a while, you start to realize that this not a suitable occupation for a self-respecting human being. That's when you realize that you need graduate students".|
|You appreciate now why we need to
have all those students. They enjoy (we believe) doing this kind of work for
their Master or PhD theses.
The figure above shows just one of the many curves produced by scores of graduate students. It shows what you get for 4 % Al in Cu "tempered" at 150 oC (302 oF) for quite a while. Note that 1000 hours equal 6 weeks. What was measured is the yield strength or hardness as we know by now.
|The Aluminum - Copper Experiment Explained|
|What we did was
hardening our Al - Cu alloy by
ageing. What happened is very clear
(and supported by much more data). It illustrates quite nicely what hardening
any metal is all about. You know, of course by now that it is all about the
obstruction of dislocation movement by
Now let's look at the data.
|For the first few hours of tempering
the tensile strength (or hardness) goes down because extremely tiny precipitates or nuclei
form. That reduces the number of obstacles a lot. For example, if If you form
agglomerates that of just three Cu atoms, you reduc the number fo obstacles
threefold,. In a volume that originally contained 90 Cu atoms for example, you
now have 30 three-atom agglomerates. Each tiny precipitate or nuclei might
obstruct dislocation movement a bit more than a single Cu atoms but since you
don't have that many obstructions any more, the total effect is less obstruction to the
onslaught of the dislocations. Look at
the analogy again.
Eventually - after about 7 hours of annealing - the precipitates grew large enough to seriously obstruct dislocation movement and the "hardness" goes up. "Seriously" means that for example a 100 Cu atom precipitate obstructs dislocation movement more than 100 single Cu atoms.
The hardness reaches a maximum after about 100 hours; obviously at this point in time we have the optimal number-size relationship for the precipitates. Around this time we may also have used up all the available copper atoms.
|If we keep at it, the hardness will go down again. That happens because now Ostwald ripening takes over. All copper atoms originally dissolved in the aluminum are used up and imprisoned in precipitates. Further growth of precipitates can only happen by the bigger ones cannibalizing the smaller ones, and that is exactly what happens. We get fewer and fewer but larger and large precipitates. Few and very large precipitates do not bother dislocations all that much, hardness goes down.|
|Of course, we can learn far more
from an analysis like that. But that involves cumbersome details and an
equation or two. The link provides for that.
Here we just note that the battle line scenario given before is rather realistic and now we even know how to deploy the troops we have in the best possible way - in a simple little war and without regard to money.
Iron is a far trickier opponent then aluminum when it comes to hardening, and it fights dirty. We also need to get to terms with it on a limited money and time budget, so we aren't done yet.
|But let's continue with looking at the results of the beautiful Al - Cu experiment and ponder some of the topics it touches upon.|
|All in all, the maximum hardness we could produce is almost three times larger than the minimum one, and that's quite an achievement. Moreover, we know exactly what is going on, and we can control it to a large degree.|
|If Ostwald ripening seems still strange, here is
a comforting thought. You can watch it happen while drinking
beer. Right after pouring the
beer consists of a liquid and foam (the head).
The head consists of many tiny bubbles formed by a thin membrane of the liquid and the gas enclosed. The beer is very unhappy with this. Its nirvana state would be what we call "flat" - no bubbles! Why? Because foam means liquid with a lot of surface area and thus unnecessary energy.
So Ostwald ripening commences. Some bubbles collapse, giving the gas they contain to others that are now bigger. And so on. Big bubbles come into being by eating up small ones (provided you let it happen before you guzzle them up). The reason for that is the same as for precipitates: the driving force is the possible gain in surface energy by reducing the surface area as much as possible.
|Isn't that great? Finally you have a
good reason to drink a lot of beer because you are actually doing science,
studying Ostwald ripening.
Since it's a complicated process when you look at the details, I recommend lots of studying. You might augment your studies with some Swiss cheese, realizing that the holes in there are precipitates of some gas that actually must have started with lots of little ones but, thanks to the second law and Ostwald ripening, developed into the few big ones you are familiar with.
|Back to beer cans. (Hey, another scientific reason to drink beer!). With all the work that produced the figure above, we now know one temperature profile that forces Aluminum plus 4 % of copper to do what we want - within the basic limits of the system.|
|It is a simple profile: Cool rapidly
to room tenpertures and then go up to the desired temperature. Keep that
temperature constant for as long as you fancy, then drop quickly to room
Simple - but there is a catch: it takes too long for the best result - about 100 hours! Far too expensive. So, maybe, we should:
|You can spend any amount of time tinkering around with optimizing beer cans, boring your female graduate students to tears. Nevertheless, you can never be sure that you found the best way to make your beer cans. So let's have another big epiphany:|
|If you have a (mathematical, of course) theory about hardening aluminum (and anything else) you could just calculate all of the above. It not only saves a lot of time and money, you also can be sure that you arrive at the best possible process - not to mention that your graduate students now can try their ken at something more challenging, like making superior steel for swords. And you have more time to study Ostwald ripening with beer, so everybody profits.|
|You have a why question? Why, for demonstrating how to outwit
the second law, did I pick an example from the boring world of aluminum and not
from the exciting world of steel ?
Well, I invoked the principle of supreme laziness.
|The iron -carbon system that we call (carbon) steel is far more complicated than the Al - Cu system. Looking at a comparable experiment for steel would have needed far more writing, which is hard work that keeps me from studying Ostwald ripening.|
|OK. Just to keep you in good humor, here is an actual and interesting steel example:|
|We have soft, low-carbon sheet-metal steel that shows the effect of ageing at room temperature. Its hardness changes ever so slowly at room temperature but after a year has passed it is substantially increased.|
|You might think that this is good. No. it isn't. Hard is not always better than soft; hard steel sheets can be quite irritating if you want to shape the stuff easily. The Aluminum foil you use to wrap your food with shouldn't be too hard, for example.|
|What has happened? First
of all, you still have some excess carbon in this iron at room temperature. Not
all of the stuff has precipitated into cementite, probably because it was
cooled too quickly. That's easy to do with thin sheets: just letting it
"sit" after hot-rolling might be sufficient.
At room temperature carbon interstitials and some other interstitial like nitrogen (N) are still a little bit mobile; look at the numbers I provided a long time ago. The carbon atoms move ever so slowly (roughly a few µm per year) until they get caught at some precipitate or in the core region of a dislocation, where they come to rest.
The net effect is that they make it more difficult for the dislocations to move when the need arrives, and that means the material is now harder.
|Now let's get back to the topic we're actually looking at. You probably forgot it by now, so let's dedicate a whole paragraph to it.|
© H. Föll (Iron, Steel and Swords script)