Mercurial > jaynes
changeset 2:afbe1fe19b36
Transcribed up to section 1.6, the first law.
author | Dylan Holmes <ocsenave@gmail.com> |
---|---|
date | Sat, 28 Apr 2012 23:06:48 -0500 |
parents | 4da2176e4890 |
children | 8f3b6dcb9add |
files | org/stat-mech.org |
diffstat | 1 files changed, 279 insertions(+), 1 deletions(-) [+] |
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1.1 --- a/org/stat-mech.org Sat Apr 28 22:03:39 2012 -0500 1.2 +++ b/org/stat-mech.org Sat Apr 28 23:06:48 2012 -0500 1.3 @@ -628,9 +628,287 @@ 1.4 ** Heat 1.5 We are now in a position to consider the results and interpretation of 1.6 a number of elementary experiments involving 1.7 +thermal interaction, which can be carried out as soon as a primitive 1.8 +thermometer is at hand. In fact these experiments, which we summarize 1.9 +so quickly, required a very long time for their first performance, and 1.10 +the essential conclusions of this Section were first arrived at only 1.11 +about 1760---more than 160 years after Galileo's invention of the 1.12 +thermometer---by Joseph Black, who was Professor of Chemistry at 1.13 +Glasgow University. Black's analysis of calorimetric experiments 1.14 +initiated by G. D. Fahrenheit before 1736 led to the first recognition 1.15 +of the distinction between temperature and heat, and prepared the way 1.16 +for the work of his better-known pupil, James Watt. 1.17 1.18 +We first observe that if two bodies at different temperatures are 1.19 +separated by walls of various materials, they sometimes maintain their 1.20 +temperature difference for a long time, and sometimes reach thermal 1.21 +equilibrium very quickly. The differences in behavior observed must be 1.22 +ascribed to the different properties of the separating walls, since 1.23 +nothing else is changed. Materials such as wood, asbestos, porous 1.24 +ceramics (and most of all, modern porous plastics like styrofoam), are 1.25 +able to sustain a temperature difference for a long time; a wall of an 1.26 +imaginary material with this property idealized to the point where a 1.27 +temperature difference is maintained indefinitely is called an 1.28 +/adiabatic wall/. A very close approximation to a perfect adiabatic 1.29 +wall is realized by the Dewar flask (thermos bottle), of which the 1.30 +walls consist of two layers of glass separated by a vacuum, with the 1.31 +surfaces silvered like a mirror. In such a container, as we all know, 1.32 +liquids may be maintained hot or cold for days. 1.33 1.34 -* Appendix 1.35 +On the other hand, a thin wall of copper or silver is hardly able to 1.36 +sustain any temperature difference at all; two bodies separated by 1.37 +such a partition come to thermal equilibrium very quickly. Such a wall 1.38 +is called /diathermic/. It is found in general that the best 1.39 +diathermic materials are the metals and good electrical conductors, 1.40 +while electrical insulators make fairly good adiabatic walls. There 1.41 +are good theoretical reasons for this rule; a particular case of it is 1.42 +given by the [[http://en.wikipedia.org/wiki/Wiedemann_franz_law][Wiedemann-Franz law]] of solid-state theory. 1.43 + 1.44 +Since a body surrounded by an adiabatic wall is able to maintain its 1.45 +temperature independently of the temperature of its surroundings, an 1.46 +adiabatic wall provides a means of thermally /isolating/ a system from 1.47 +the rest of the universe; it is to be expected, therefore, that the 1.48 +laws of thermal interaction between two systems will assume the 1.49 +simplest form if they are enclosed in a common adiabatic container, 1.50 +and that the best way of carrying out experiments on thermal 1.51 +peroperties of substances is to so enclose them. Such an apparatus, in 1.52 +which systems are made to interact inside an adiabatic container 1.53 +supplied with a thermometer, is called a /calorimeter/. 1.54 + 1.55 +Let us imagine that we have a calorimeter in which there is initially 1.56 +a volume $V_W$ of water at a temperature $t_1$, and suspended above it 1.57 +a volume $V_I$ of some other substance (say, iron) at temperature 1.58 +$t_2$. When we drop the iron into the water, they interact thermally 1.59 +(and the exact nature of this interaction is one of the things we hope 1.60 +to learn now), the temperature of both changing until they are in 1.61 +thermal equilibrium at a final temperature $t_0$. 1.62 + 1.63 +Now we repeat the experiment with different initial temperatures 1.64 +$t_1^\prime$ and $t_2^\prime$, so that a new equilibrium is reached at 1.65 +temperature $t_0^\prime$. It is found that, if the temperature 1.66 +differences are sufficiently small (and in practice this is not a 1.67 +serious limitation if we use a mercury thermometer calibrated with 1.68 +uniformly spaced degree marks on a capillary of uniform bore), then 1.69 +whatever the values of $t_1^\prime$, $t_2^\prime$, $t_1$, $t_2$, the 1.70 +final temperatures $t_0^\prime$, $t_0$ will adjust themselves so that 1.71 +the following relation holds: 1.72 + 1.73 +\begin{equation} 1.74 +\frac{t_2 - t_0}{t_0 - t_1} = \frac{t_2^\prime - 1.75 +t_0^\prime}{t_0^\prime - t_1^\prime} 1.76 +\end{equation} 1.77 + 1.78 +in other words, the /ratio/ of the temperature changes of the iron and 1.79 +water is independent of the initial temperatures used. 1.80 + 1.81 +We now vary the amounts of iron and water used in the calorimeter. It 1.82 +is found that the ratio (1-8), although always independent of the 1.83 +starting temperatures, does depend on the relative amounts of iron and 1.84 +water. It is, in fact, proportional to the mass $M_W$ of water and 1.85 +inversely proportional to the mass $M_I$ of iron, so that 1.86 + 1.87 +\begin{equation} 1.88 +\frac{t_2-t_0}{t_0-t_1} = \frac{M_W}{K_I M_I} 1.89 +\end{equation} 1.90 + 1.91 +where $K_I$ is a constant. 1.92 + 1.93 +We next repeat the above experiments using a different material in 1.94 +place of the iron (say, copper). We find again a relation 1.95 + 1.96 +\begin{equation} 1.97 +\frac{t_2-t_0}{t_0-t_1} = \frac{M_W}{K_C \cdot M_C} 1.98 +\end{equation} 1.99 + 1.100 +where $M_C$ is the mass of copper; but the constant $K_C$ is different 1.101 +from the previous $K_I$. In fact, we see that the constant $K_I$ is a 1.102 +new physical property of the substance iron, while $K_C$ is a physical 1.103 +property of copper. The number $K$ is called the /specific heat/ of a 1.104 +substance, and it is seen that according to this definition, the 1.105 +specific heat of water is unity. 1.106 + 1.107 +We now have enough experimental facts to begin speculating about their 1.108 +interpretation, as was first done in the 18th century. First, note 1.109 +that equation (1-9) can be put into a neater form that is symmetrical 1.110 +between the two substances. We write $\Delta t_I = t_0 - t_2$, $\Delta 1.111 +t_W = t_0 - t_1$ for the temperature changes of iron and water 1.112 +respectively, and define $K_W \equiv 1$ for water. Equation (1-9) then 1.113 +becomes 1.114 + 1.115 +\begin{equation} 1.116 +K_W M_W \Delta t_W + K_I M_I \Delta t_I = 0 1.117 +\end{equation} 1.118 + 1.119 +The form of this equation suggests a new experiment; we go back into 1.120 +the laboratory, and find $n$ substances for which the specific heats 1.121 +\(\{K_1,\ldots K_n\}\) have been measured previously. Taking masses 1.122 +\(\{M_1, \ldots, M_n\}\) of these substances, we heat them to $n$ 1.123 +different temperatures \(\{t_1,\ldots, t_n\}\) and throw them all into 1.124 +the calorimeter at once. After they have all come to thermal 1.125 +equilibrium at temperature $t_0$, we find the differences $\Delta t_j 1.126 += t_0 - t_j$. Just as we suspected, it turns out that regardless of 1.127 +the $K$'s, $M$'s, and $t$'s chosen, the relation 1.128 +\begin{equation} 1.129 +\sum_{j=0}^n K_j M_j \Delta t_j = 0 1.130 +\end{equation} 1.131 +is always satisfied. This sort of process is an old story in 1.132 +scientific investigations; although the great theoretician Boltzmann 1.133 +is said to have remarked: \ldquo{}Elegance is for tailors \rdquo{}, it 1.134 +remains true that the attempt to reduce equations to the most 1.135 +symmetrical form has often suggested important generalizations of 1.136 +physical laws, and is a great aid to memory. Witness Maxwell's 1.137 +\ldquo{}displacement current\rdquo{}, which was needed to fill in a 1.138 +gap and restore the symmetry of the electromagnetic equations; as soon 1.139 +as it was put in, the equations predicted the existence of 1.140 +electromagnetic waves. In the present case, the search for a rather 1.141 +rudimentary form of \ldquo{}elegance\rdquo{} has also been fruitful, 1.142 +for we recognize that (1-12) has the standard form of a /conservation 1.143 +law/; it defines a new quantity which is conserved in thermal 1.144 +interactions of the type just studied. 1.145 + 1.146 +The similarity of (1-12) to conservation laws in general may be seen 1.147 +as follows. Let $A$ be some quantity that is conserved; the $i$th 1.148 +system has an amount of it $A_i$. Now when the systems interact such 1.149 +that some $A$ is transferred between them, the amount of $A$ in the 1.150 +$i$th system is changed by a net amount \(\Delta A_i = (A_i)_{final} - 1.151 +(A_i)_{initial}\); and the fact that there is no net change in the 1.152 +total amount of $A$ is expressed by the equation \(\sum_i \Delta 1.153 +A_i = 0$. Thus, the law of conservation of matter in a chemical 1.154 +reaction is expressed by \(\sum_i \Delta M_i = 0\), where $M_i$ is the 1.155 +mass of the $i$th chemical component. 1.156 + 1.157 +what is this new conserved quantity? Mathematically, it can be defined 1.158 +as $Q_i = K_i\cdot M_i cdot t_i; whereupon (1-12) becomes 1.159 + 1.160 +\begin{equation} 1.161 +\sum_i \Delta Q_i = 0 1.162 +\end{equation} 1.163 + 1.164 +and at this point we can correct a slight quantitative inaccuracy. As 1.165 +noted, the above relations hold accurately only when the temperature 1.166 +differences are sufficiently small; i.e., they are really only 1.167 +differential laws. On sufficiently accurate measurements one find that 1.168 +the specific heats $K_i$ depend on temperature; if we then adopt the 1.169 +integral definition of $\Delta Q_i$, 1.170 +\begin{equation} 1.171 +\Delta Q_i = \int_{t_{i}}^{t_0} K_i(t) M_i dt 1.172 +\end{equation} 1.173 + 1.174 +the conservation law (1-13) will be found to hold in calorimetric 1.175 +experiments with liquids and solids, to any accuracy now feasible. And 1.176 +of course, from the manner in which the $K_i(t)$ are defined, this 1.177 +relation will hold however our thermometers are calibrated. 1.178 + 1.179 +Evidently, the stage is now set for a \ldquo{}new\rdquo{} physical 1.180 +theory to account for these facts. In the 17th century, both Francis 1.181 +Bacon and Isaac Newton had expressed their opinions that heat was a 1.182 +form of motion; but they had no supporting factual evidence. By the 1.183 +latter part of the 18th century, one had definite factual evidence 1.184 +which seemed to make this view untenable; by the calorimetric 1.185 +\ldquo{}mixing\rdquo{} experiments just described, Joseph Black had 1.186 +recognized the distinction between temperature $t$ as a measure of 1.187 +\ldquo{}hotness\rdquo{}, and heat $Q$ as a measure of /quantity/ of 1.188 +something, and introduced the notion of heat capacity. He also 1.189 +recognized the latent heats of freezing and vaporization. To account 1.190 +for the conservation laws thus discovered, the theory then suggested 1.191 +itself, naturally and almost inevitably, that heat was /fluid/, 1.192 +indestructable and uncreatable, which had no appreciable weight and 1.193 +was attracted differently by different kinds of matter. In 1787, 1.194 +Lavoisier invented the name \ldquo{}caloric\rdquo{} for this fluid. 1.195 + 1.196 +Looking down today from our position of superior knowledge (i.e., 1.197 +hindsight) we perhaps need to be reminded that the caloric theory was 1.198 +a perfectly respectable scientific theory, fully deserving of serious 1.199 +consideration; for it accounted quantitatively for a large body of 1.200 +experimental fact, and made new predictions capable of being tested by 1.201 +experiment. 1.202 + 1.203 +One of these predictions was the possibility of accounting for the 1.204 +thermal expansion of bodies when heated; perhaps the increase in 1.205 +volume was just a measure of the volume of caloric fluid 1.206 +absorbed. This view met with some disappointment as a result of 1.207 +experiments which showed that different materials, on absorbing the 1.208 +same quantity of heat, expanded by different amounts. Of course, this 1.209 +in itself was not enough to overthrow the caloric theory, because one 1.210 +could suppose that the caloric fluid was compressible, and was held 1.211 +under different pressure in different media. 1.212 + 1.213 +Another difficulty that seemed increasingly serious by the end of the 1.214 +18th century was the failure of all attempts to weigh this fluid. Many 1.215 +careful experiments were carried out, by Boyle, Fordyce, Rumford and 1.216 +others (and continued by Landolt almost into the 20th century), with 1.217 +balances capable of detecting a change of weight of one part in a 1.218 +million; and no change could be detected on the melting of ice, 1.219 +heating of substances, or carrying out of chemical reactions. But even 1.220 +this is not really a conclusive argument against the caloric theory, 1.221 +since there is no /a priori/ reason why the fluid should be dense 1.222 +enough to weigh with balances (of course, we know today from 1.223 +Einstein's $E=mc^2$ that small changes in weight should indeed exist 1.224 +in these experiments; but to measure them would require balances about 1.225 +10^7 times more sensitive than were available). 1.226 + 1.227 +Since the caloric theory derives entirely from the empirical 1.228 +conservation law (1-33), it can be refuted conclusively only by 1.229 +exhibiting new experimental facts revealing situations in which (1-13) 1.230 +is /not/ valid. The first such case was [[http://www.chemteam.info/Chem-History/Rumford-1798.html][found by Count Rumford (1798)]], 1.231 +who was in charge of boring cannon in the Munich arsenal, and noted 1.232 +that the cannon and chips became hot as a result of the cutting. He 1.233 +found that heat could be produced indefinitely, as long as the boring 1.234 +was continued, without any compensating cooling of any other part of 1.235 +the system. Here, then, was a clear case in which caloric was /not/ 1.236 +conserved, as in (1-13); but could be created at will. Rumford wrote 1.237 +that he could not conceive of anything that could be produced 1.238 +indefinitely by the expenditure of work, \ldquo{}except it be /motion/\rdquo{}. 1.239 + 1.240 +But even this was not enough to cause abandonment of the caloric 1.241 +theory; for while Rumford's observations accomplished the negative 1.242 +purpose of showing that the conservation law (1-13) is not universally 1.243 +valid, they failed to accomplish the positive one of showing what 1.244 +specific law should replace it (although he produced a good hint, not 1.245 +sufficiently appreciated at the time, in his crude measurements of the 1.246 +rate of heat production due to the work of one horse). Within the 1.247 +range of the original calorimetric experiments, (1-13) was still 1.248 +valid, and a theory successful in a restricted domain is better than 1.249 +no theory at all; so Rumford's work had very little impact on the 1.250 +actual development of thermodynamics. 1.251 + 1.252 +(This situation is a recurrent one in science, and today physics offers 1.253 +another good example. It is recognized by all that our present quantum 1.254 +field theory is unsatisfactory on logical, conceptual, and 1.255 +mathematical grounds; yet it also contains some important truth, and 1.256 +no responsible person has suggested that it be abandoned. Once again, 1.257 +a semi-satisfactory theory is better than none at all, and we will 1.258 +continue to teach it and to use it until we have something better to 1.259 +put in its place.) 1.260 + 1.261 +# what is "the specific heat of a gas at constant pressure/volume"? 1.262 +# changed t for temperature below from capital T to lowercase t. 1.263 +Another failure of the conservation law (1-13) was noted in 1842 by 1.264 +R. Mayer, a German physician, who pointed out that the data already 1.265 +available showed that the specific heat of a gas at constant pressure, 1.266 +C_p, was greater than at constant volume $C_v$. He surmised that the 1.267 +difference was due to the work done in expansion of the gas against 1.268 +atmospheric pressure, when measuring $C_p$. Supposing that the 1.269 +difference $\Delta Q = (C_p - C_v)\Delta t$ calories, in the heat 1.270 +required to raise the temperature by $\Delta t$ was actually a 1.271 +measure of amount of energy, he could estimate from the amount 1.272 +$P\Delta V$ ergs of work done the amount of mechanical energy (number 1.273 +of ergs) corresponding to a calorie of heat; but again his work had 1.274 +very little impact on the development of thermodynamics, because he 1.275 +merely offered this notion as an interpretation of the data without 1.276 +performing or suggesting any new experiments to check his hypothesis 1.277 +further. 1.278 + 1.279 +Up to the point, then, one has the experimental fact that a 1.280 +conservation law (1-13) exists whenever purely thermal interactions 1.281 +were involved; but in processes involving mechanical work, the 1.282 +conservation law broke down. 1.283 + 1.284 +** The First Law 1.285 + 1.286 + 1.287 + 1.288 +* COMMENT Appendix 1.289 1.290 | Generalized Force | Generalized Displacement | 1.291 |--------------------+--------------------------|