The Thermodynamics of Beards

When I was an undergraduate studying physics, my physics supervisor (who happens to be a regular contributor to the comments on this blog) introduced me to thermodynamics by explaining that Ludwig Boltzmann committed suicide in 1906, as did Paul Ehrenfest in 1933. Now it was my turn to study what had driven them both to take their own lives.

I didn’t think this was the kind of introduction likely to inspire a joyful curiosity in the subject, but it probably wasn’t the reason why I found the subject as difficult as I did. I thought it was a hard subject because it seemed to me to possess arbitrary rules that didn’t emerge from a simpler underlying principle, but simply had to be memorized. Lurking somewhere under it was obviously something statistical, but what it was or how it worked was never made clear. I was frequently told that the best thing to do was just memorize all the different examples given and not try to understand where it all came from. I tried doing this but, partly because I have a very poor memory, I didn’t so very well in the final examination on this topic. I was prejudiced against it for years afterwards.

Actually, now I have grown to like thermodynamics as a subject and have read quite a bit about its historical development. The field of thermodynamics is usually presented to students as a neat and tidy system of axioms and definitions. The resulting laws are written in the language of idealised gases, perfect mechanical devices and reversible equilibrium paths but, despite this, have many applications in realistic practical situations. What is particularly interesting about these laws is that it took a very long time indeed to establish them even at this macroscopic level. The deeper understanding of their origin in the microphysics of atoms and molecules took even longer and was an even more difficult journey.   I thought it might be  fun to celebrate  the tangled history of this fascinating subject, at least for a little while.  Unlike quantum physics and relativity, thermodynamics is not regarded as a very “glamorous” part of science by the general public, but it did occupy the minds of the greatest physicists of the nineteenth century, and I think the story deserves to be better appreciated. I don’t have space to give a complete account, so I apologize in advance for the omissions.

I thought it would also be fun to show pictures of the principal characters. As you’ll see, after  a very clean-shaven start, the history of thermodynamics is dominated by a succession of rather splendid beards…

I’ll start the story with Nicolas Léonard Sadi Carnot (left), who  was born in 1796. His family background was, to say the least, unusual. His father Lasare was known as the “Organizer of Victory” for the Revolutionary Army in 1794 and subsequently became Napoleon’s minister of war. Against all expectations he quit politics in 1807 and became a mathematician. Sadi had a brother, by the splendid name of Hippolyte, who was also a politician and whose son became president of France. Sadi himself was educated partly by his father and partly at the Ecole Polytecnhique. He served in the army as an engineer and was eventually promoted to Captain. He left the army in 1828, only to die of cholera in 1832 during an epidemic in Paris.

Carnot’s work on the theory of “heat engines” was astonishingly original and eventually had enormous impact, essentially creating the new science of thermodynamics, but he only published one paper before his untimely death and it attracted little attention during his lifetime. Reflections on the Motive Power of Fire appeared in 1824, but its importance was not really recognized until 1849, when it was read by William Thomson (later Lord Kelvin) who, together Rudolf Clausius, made it more widely known.

In the late 18th century, Britain was in the grip of an industrial revolution largely generated by the use of steam power. These engines had been invented by the pragmatic British, but the theory by which they worked was pretty much non-existent. Carnot realised that steam-driven devices in use at the time were horrendously inefficient. As a nationalist, he hoped that by thinking about the underlying principles of heat and energy he might be able to give his native France a competitive edge over perfidious Albion. He thought about the problem of heat engines in the most general terms possible, even questioning whether there might be an alternative to steam as the best possible “working substance”. Despite the fact that he employed many outdated concepts, including the so-called caloric theory of heat, Carnot’s paper was full of brilliant insights. In particular he considered the behaviour of an idealized friction-free engine in which the working substance moves from a heat source to a heat sink in a series of small equilibrium steps so that the entire process is reversible. The changes of pressure and volume involved in such a process are now known as a Carnot cycle.

By remarkably clear reasoning, Carnot was able to prove a famous theorem that the efficiency of such a cycle depends only on the temperature Tin of the heat source and the temperature Tout. He showed that the maximum fraction of the heat available to be used to do mechanical work is independent of the working substance and is equal to (Tin-Tout)/Tout; this is called Carnot’s theorem. Carnot’s results were probably considered too abstract to be of any use to engineers, but they contain ideas that are linked with the First Law of Thermodynamics, and they eventually led Clausius and Thomson independently to the statement of the Second Law discussed below.

James Prescott Joule (right) was growing up in a wealthy brewing family. He was born in 1818 and was educated at home by none other than John Dalton. He became interested in science and soon started doing experiments in a laboratory near the family brewery. He was a skilful practical physicist and was able to measure the heat and temperature changes involved in various situations. Between 1837 and 1847 he established the basic principle that heat and other forms of energy (such as mechanical work) were equivalent and that, when all forms are included, energy is conserved. Joule measured the amount of mechanical work required to produce a given amount of heat in 1843, by studying the heat released in water by the rotation of paddles powered by falling weights. The SI unit of energy is named in his honour.

William Thomson, 1st Baron Kelvin of Largs, was born in 1824 and came to dominate British physics throughout the second half of the 19th  century. He was extremely prolific, writing over 600 research papers and several books. No-one since has managed to range so widely and so successfully across the realm of natural sciences. He was also unusually generous with his ideas (perhaps because he had so many), and in giving credit to other scientists, such as Carnot.  He wasn’t entirely enlightened, however: he was a vigorous opponent of the admission of women to the  University.

Kelvin worked on many theoretical aspects of physics, but was also extremely practical. He directed the first successful transatlantic cable telegraph project, and his house in Glasgow was one of the first to be lit by electricity. Unusually among physicists he became wealthy through his scientific work. One can dream.

One of the keys to Kelvin’s impact on science in Britain was that immediately after graduating from Cambridge in 1845 he went to work in Paris for a year. This opened his eyes to the much more sophisticated mathematical approaches being used by physicists on the continent. British physics, especially at Cambridge, had been held back by an excessive reverence for the work of Newton and the rather cumbersome form of calculus (called “fluxions”) it had inherited from him. Much of Kelvin’s work on theoretical topics used the modern calculus which had been developed in mainland Europe. More specifically, it was during this trip to Paris that he heard of the paper by Carnot, although it took him another three years to get his hands on a copy. When he returned from Paris in 1846, the young William Thomson became Professor of Natural Philosophy at Glasgow University, a post he held for an astonishing 53 years.

Initially inspired by Carnot’s work, Kelvin became one of the most important figures in the development of the theory of heat. In 1848 he proposed an absolute scale of temperature now known as the Kelvin or thermodynamic scale, which practically corresponds with the Celsius scale except with an offset such that the triple point of water, at zero degrees Celsius, is at 273.16 Kelvin.  He also worked with Joule on experiments concerning heat flow.

At around the same time as Kelvin, another prominent character in the story of thermodynamics was playing his part. Rudolf Clausius (right) was born in 1822. His father was a Prussian pastor and owner of a small school that the young Rudolf attended. He later went to university in Berlin to study history, but switched to science. He was constantly short of money, which meant that it took him quite a long time to graduate but he eventually ended up as a professor of physics, first in Zürich and then later in Wurzburg and Bonn. During the Franco-Prussian war, he and his students set up a volunteer ambulance service and during the course of its operations, Rudolf Clausius was badly wounded.

By the 1850s, thanks largely to the efforts of Kelvin, Carnot’s work was widely recognized throughout Europe. Carnot had correctly realised that in a steam engine, heat “moves” as the steam descends from a higher temperature to a lower one. He, however, envisaged that this heat moved through the engine intact.  On the other hand, the work of Joule had established The First law of Thermodynamics, which states that heat is actually lost in this process, or more precisely heat is converted into mechanical work. Clausius was troubled by the apparent conflict between the views of Carnot and Joule, but eventually realised that they could be reconciled if one could assume that heat does not pass spontaneously from a colder to a hotter body. This was the original statement of what has become known as the Second Law of Thermodynamics.  The following year, Kelvin came up with a different expression of essentially the same law.  Clausius further developed the idea that heat must tend to dissipate and in 1865 he introduced the term “entropy”  as a measure of the amount of heat gained or lost by a body divided by its absolute temperature. An equivalent statement of the Second Law is that the entropy of an isolated system can never decrease: it can only either increase or remain constant. This principle was intensely controversial at the time, but Kelvin and Maxwell fought vigorously in its defence, and it was eventually accepted into the canon of Natural Law.

So far in this brief historical diversion, I have focussed on thermodynamics at a macroscopic level, in the form that eventually emerged as the laws of thermodynamics presented in the previous section. During roughly the same period, however, a parallel story was unfolding that revolved around explaining the macroscopic behaviour of matter in terms of the behaviour of its microscopic components. The goal of this programme was to understand quantitative measures such as temperature and pressure in terms of related quantities describing individual atoms or molecules. I’ll end this bit of history with a brief description of three of the most important contributors to this strand.

James_clerk_maxwell

James Clerk Maxwell (above) was probably the greatest physicist of the nineteenth century, and although he is most celebrated for his phenomenal work on the unified theory of electricity and magnetism, he was also a great pioneer in the kinetic theory of gases, He was born in 1831 and went to school at the Edinburgh academy, which was a difficult experience for him because he had a country accent and invariably wore home-made clothes that made him stand out among the privileged town-dwellers who formed the bulk of the school population. Aged 15, he invented a method of drawing curves using string and drawing pins as a kind of generalization of the well-known technique of drawing an ellipse. This work was published in the Proceedings of the Royal Society of Edinburgh in 1846, a year before Maxwell went to University. After a spell at Edinburgh he went to Cambridge in 1850; while there he won the prestigious Smith’s prize in 1854. He subsequently obtained a post in Aberdeen at Marischal College where he married the principal’s daughter, but was then made redundant. In 1860 he moved to London but when his father died in 1865 he resigned his post at King’s college and became a gentleman farmer doing scientific research in his spare time. In 1874 he was persuaded to move to Cambridge as the first Cavendish Professor of Experimental Physics, charged with the responsibility of setting up the now-famous Cavendish laboratory. He contracted cancer five years later and died, aged 48, in 1879.

Maxwell’s contributions to the kinetic theory of gases began by building on the idea, originally due to Daniel Bernoulli, that a gas consists of molecules in constant motion colliding with each other and with the walls of whatever container is holding it. Rudolf Clausius had already realised that although the gas molecules travel very fast, gases diffuse into each other only very slowly. He deduced, correctly, that molecules must only travel a very short distance between collisions. From about 1860, Maxwell started to work on the application of statistical methods to this general picture. He worked out the probability distribution of molecular velocities in a gas in equilibrium at a given temperature; Boltzmann (see below) independently derived the same result. Maxwell showed how the distribution depends on temperature and also proved that heat must be stored in a gas in the form of kinetic energy of the molecules, thus establishing a microscopic version of the first law of thermodynamics. He went on to explain a host of experimental properties such as viscosity, diffusion and thermal conductivity using this theory.

Maxwell was lucky that he was able to make profound intellectual discoveries without apparently suffering from significant mental strain. Unfortunately, the same could not be said of Ludwig Eduard Boltzmann, who was born in 1844 and grew up in the Austrian towns of Linz and Wels, where his father was employed as a tax officer. He received his doctorate from the University of Vienna in 1866 and subsequently held a series of professorial appointments at Graz, Vienna, Munich and Leipzig. Throughout his life he suffered from bouts of depression which worsened when he was subjected to sustained attack from the Vienna school of positivist philosophers, who derided the idea that physical phenomena could be explained in terms of atoms. Despite this antagonism, he taught many students who went on to become very distinguished and he also had a very wide circle of friends. In the end, though, the lack of acceptance of his work got him so depressed that he committed suicide in 1906. Max Planck arranged for his gravestone to be marked with “S=klogW”, which is now known as Boltzmann’s law; the constant k is called Boltzmann’s constant.

The final member of the cast of characters in this story is Josiah Willard Gibbs (left). He born in 1839 and received his doctorate from Yale University in 1863, gaining only the second PhD ever to be awarded in the USA.  After touring Europe for a while he returned to Yale in 1871 to become a professor, but he received no salary for the first nine years of this appointment. The university rules at that time only allowed salaries to be paid to staff in need of money; having independent means, Gibbs was apparently not entitled to a salary. Gibbs was a famously terrible teacher and few students could make any sense of his lectures (not a rare occurence amongst those trying to learn thermodynamics). His research papers are written in a very obscure style which makes it easy to believe he found it difficult to express himself in the lecture theatre. Gibbs actually founded the field of chemical thermodynamics, but few chemists understood his work while he was still alive. His great contribution to statistical mechanics was likewise poorly understood. It was only in the 1890s when his works were translated into German that his achievements became more widely recognised. Both Planck and Einstein held him in very high regard, but even they found his work difficult to understand. He died in 1903.

So there you are. The only one who didn’t have a beard was French and called Sadi. ’nuff said.

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6 Responses to “The Thermodynamics of Beards”

  1. Anton Garrett Says:

    Nice summary Peter. I hope you will write Part II about how (and how not) to bring the macroscopic and microscopic descriptions together…
    Anton

  2. telescoper Says:

    Anton, that’s the really interesting part…but I think it will be a while before I get time to tackle such a challenging topic!

  3. Bryn Jones Says:

    This introduction to the history of thermodynamics is welcome and interesting.

    I failed to understand thermodynamics as an undergraduate, and assumed that it was because I was rather stupid. I constructed arguments in my head rather like Maxwell’s demons, and could not reconcile thermodynamic concepts with an expanding Universe. It was only much later that I found that these objections were not entirely stupid and that they inform our understanding of the subject (as you mentioned in your earlier posting about the Big Bang). It is likely that most undergraduates find thermodynamics challenging, and perhaps we should consider that healthy.

  4. […] arose from the developments of kinetic theory and statistical mechanics that I discussed briefly in a previous post. Inspired by such luminaries as James Clerk Maxwell and Ludwig Boltzmann, physicists had inexorably […]

  5. […] For the physicists among my readers here is an old post of mine about the role of beards in the development of […]

  6. […] a personal level, acknowledging the fundamental importance of beards in the history of Physics, I have produced a detailed three-point guide on Beard Growth for members of my own School, and we […]

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