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The following is a thought experiment. Nothing written here should be construed as instructions for practical action. This is not a homework problem.
You go to your freezer, take out an ice cube, and put it in an experimental fluid of your choice. Some of the choicest fluids for this experiment are made along the banks of glens in Scotland. A scientist often feels compelled to repeat an experiment many times to be sure that the results are dependable. If you do so in this case, you might not be able to remember the results.
Here is what you observe. The fluid starts out at room temperature. The ice is initially at the temperature of the freezer, say, 260 K or -13°C. At first the ice warms up, cooling the fluid. But then, when its temperature reaches 273 K or 0°C something happens that is both extraordinary and dramatic. The ice refuses to get any warmer. Whereas just before it had no difficulty raising its temperature as it absorbed heat, it now absolutely refuses to warm the slightest bit more. Instead it undergoes a catastrophic change in its microscopic state. As it absorbs more heat from its surroundings, the molecules separate from their solid crystal structure. The ice melts into water. The whole profound transformation takes place without permitting any change in temperature until it is completely finished. If that were not the case, you wouldn’t cool your drinks with ice. You might as well throw cold rocks in them.
In Chapter 1 we made a truly remarkable simplification of nature. For a body of a given U, N and V it's not necessary to know what each of its atoms is doing. If we allow the body to come to equilibrium, all the microscopic information necessary to specify its macroscopic state is contained in the value of a single variable, the entropy. In this chapter we shall explore some of the consequences of that profound insight.
If we know explicitly the equation U = U(S, V, N), then we have enough information to find anything we want. For this reason S, V and N are said to be the proper variables of the energy U. We have already had some examples of how information can be extracted from this equation, and we shall have some more (Problems 2.5 and 2.7). In reality the equation is hardly ever known explicitly for any real system, but the fact that it exists in principle – which was the point of the first chapter – is what we wish to exploit.
There are seven thermodynamic variables, and these can be grouped into classes in various ways. One way is to assemble them into conjugate pairs. Each pair, when multiplied together, has the units of energy. They can also be classified as either extensive or intensive. Both are shown in Table 2.1.
The origin and meaning of the first and second laws
Of all the tales in the repertory of human folklore, one of the best may be one that is hardly ever told. It is the epic saga of the second law of thermodynamics. The second law was born in an attempt to improve the steam engine, and it went on to predict the ultimate fate of the Universe. It captured the popular imagination, defined the meaning of time, and led to the discovery of quantum mechanics. It was born, like some mythical beast, before its putative mother, the first law of thermodynamics.
Before we get swept away by the mighty tide of these powerful laws, let us remind ourselves that we already know everything there is to know about what they say and why they are true. The first law expresses, in a special way, the conservation of energy. We examined it at some length earlier. The second law says essentially that the entropy of an isolated system increases until it can get no larger. We’ve already seen that that’s true. What we have to say here is therefore mere elaboration.
Before the middle of the nineteenth century, it was believed that heat was a fluid, called caloric, which could flow fromone body to another. That view differed from our present understanding in that each body was thought to possess a definite amount of caloric, which, being a fluid, could neither be created nor be destroyed. It was a successful theory, but it wasn’t quite right.
Encouraged to share his memories of Michael Faraday (1791–1867), John Hall Gladstone (1827–1902) published in 1872 this short work about his late friend's life and career. Faraday's successor as Fullerian Professor of Chemistry at the Royal Institution, Gladstone discusses how Faraday approached science, and the value of his discoveries. Offering informed insights into Faraday's character, Gladstone includes a number of extracts from personal letters. The work also includes a translation of part of the eulogy given by Jean-Baptiste Dumas at the Académie des Sciences, as well as an anonymous poem honouring Faraday and published in Punch shortly after his death. An appendix lists the numerous learned societies to which Faraday belonged. Also reissued in this series are The Life and Letters of Faraday (1870), compiled by Henry Bence Jones, and John Tyndall's Faraday as a Discoverer (1868).
First published in 1868, soon after the death of Michael Faraday (1791–1867), this short work assesses the discoveries made by a humble bookbinder who became one of the foremost scientific investigators of the nineteenth century. Eminently qualified, John Tyndall (1820–93), who received Faraday's support in taking up the professorship of natural philosophy at the Royal Institution in 1853, gives an informed appraisal of a remarkable scientific career. The protégé of Sir Humphry Davy, Faraday went on to carry out pioneering work in the fields of electromagnetism, diamagnetism and electrolysis. Tyndall focuses here on Faraday's research, describing his influences and how he approached his investigations, although insights into his character are also incorporated: 'Underneath his sweetness and gentleness was the heat of a volcano.' Also reissued in this series are The Life and Letters of Faraday (1870), compiled by Henry Bence Jones, and John Hall Gladstone's Michael Faraday (1872).
The Austrian scientist Ernst Mach (1838–1916) carried out work of importance in several fields of enquiry, including physics, physiology and psychology. In this short work, first published in German in 1872 and translated here into English in 1911 by Philip E. B. Jourdain (1879–1919) from the 1909 second edition, Mach discusses the formulation of one of science's most fundamental theories. He provides his interpretation of the principle of the conservation of energy, claiming its foundations are not in mechanical physics. Mach's 1868 work on the definition of mass - one of his most significant contributions to mechanics - has been incorporated here. His perspective on the topic as a whole remains relevant to those interested in the history of science and the theory of knowledge. Also reissued in this series in English translation are Mach's The Science of Mechanics (1893) and Popular Scientific Lectures (1895).
Striving to explore the subject in as simple a manner as possible, this book helps readers understand the elusive concept of entropy. Innovative aspects of the book include the construction of statistical entropy from desired properties, the derivation of the entropy of classical systems from purely classical assumptions, and a statistical thermodynamics approach to the ideal Fermi and ideal Bose gases. Derivations are worked through step-by-step and important applications are highlighted in over 20 worked examples. Around 50 end-of-chapter exercises test readers' understanding. The book also features a glossary giving definitions for all essential terms, a time line showing important developments, and list of books for further study. It is an ideal supplement to undergraduate courses in physics, engineering, chemistry and mathematics.
Sir James Prescott Joule (1818–1889) became one of the most significant physicists of the nineteenth century, although his original interest in science was as a hobby and for practical business purposes. The son of a brewer, he began studying heat while investigating how to increase the efficiency of electric motors. His discovery of the relationship between heat and energy contributed to the discovery of the conservation of energy and the first law of thermodynamics. Volume 2 of his collected papers, published in 1887, contains those which he co-authored with other noted physicists, such as Scoresby, Playfair and William Thomson, later Lord Kelvin. Because he was based in Manchester, and was not an academic, Joule's work was at first ignored by the scientific establishment, but Thomson's approval helped him gain acceptance. His joint work with Thomson on thermodynamics was fundamental to the development of significant areas of twentieth-century physics.
Based around a series of real-life scenarios, this engaging introduction to statistical reasoning will teach you how to apply powerful statistical, qualitative and probabilistic tools in a technical context. From analysis of electricity bills, baseball statistics, and stock market fluctuations, through to profound questions about physics of fermions and bosons, decaying nuclei, and climate change, each chapter introduces relevant physical, statistical and mathematical principles step-by-step in an engaging narrative style, helping to develop practical proficiency in the use of probability and statistical reasoning. With numerous illustrations making it easy to focus on the most important information, this insightful book is perfect for students and researchers of any discipline interested in the interwoven tapestry of probability, statistics, and physics.