New trends in physics teaching, v.4; The ... - unesdoc - Unesco
New trends in physics teaching, v.4; The ... - unesdoc - Unesco
New trends in physics teaching, v.4; The ... - unesdoc - Unesco
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<strong>New</strong> Trends <strong>in</strong> Physics Teach<strong>in</strong>g IV<br />
to deal simply and effectively with statistical arguments - this <strong>in</strong>volves choos<strong>in</strong>g the best systems<br />
to consider, the k<strong>in</strong>d of statistics to emphasize and the mathematical resources to use; (4) how to<br />
trade rigour aga<strong>in</strong>st <strong>in</strong>tuitive understand<strong>in</strong>g (and work<strong>in</strong>g out what the latter means <strong>in</strong> this context);<br />
and (5) just what physical systems, or types of systems, to emphasize (eng<strong>in</strong>es, electrochemical<br />
cells, vapours etc.).<br />
Feynman shows that he is aware of many of these problems: ‘it is a difficult subject and the<br />
best way to learn it is to do it slowly. <strong>The</strong> first th<strong>in</strong>g is to get some idea, more or less, of what<br />
ought to happen <strong>in</strong> different circumstances, and then later. . . we wil formulate it better.’ On the<br />
macroscopic - microscopic dilemma: ‘<strong>The</strong> deepest understand<strong>in</strong>g. . . comes. . . from understand<strong>in</strong>g<br />
the actual mach<strong>in</strong>ery underneath, and that is what we shall do: we shall take the atomic<br />
viewpo<strong>in</strong>t from the beg<strong>in</strong>n<strong>in</strong>g, and use it to understand the properties of matter and the laws of<br />
thermodynamics.’ On the classical/quantum dilemma (what statistics to use) ‘. . . many th<strong>in</strong>gs<br />
that we wil deduce by classical <strong>physics</strong> wil be fundamentally <strong>in</strong>correct. . . however, we shall<br />
<strong>in</strong>dicate <strong>in</strong> every case when a result is <strong>in</strong>correct.’<br />
Feynman offers an important <strong>in</strong>sight <strong>in</strong>to this last dilemma when he writes: ‘It turns out that. . .<br />
although most problems are more difficult <strong>in</strong> quantum mechanics than <strong>in</strong> classical mechanics,<br />
problems <strong>in</strong> statistical mechanics are much easier <strong>in</strong> quantum theory.’ <strong>The</strong> reason is that <strong>in</strong><br />
quantum theory one can count: states become discrete <strong>in</strong>stead of cont<strong>in</strong>uous, so that <strong>in</strong>tegrals<br />
turn <strong>in</strong>to addition sums.<br />
Feynman’s decisions about many dilemmas are clear. He firmly emphasizes microscopic <strong>in</strong>terpretations.<br />
His statistical arguments are as simple as they can be made: no permutations or<br />
comb<strong>in</strong>ations are used at all. All the arguments concern Maxwell-Boltzmann statistics, though<br />
he takes opportunities to demonstrate the failure of classical statistics. He chooses a clear focus<br />
for argument <strong>in</strong> the Boltzmann factor, a choice enabl<strong>in</strong>g him to illustrate the wide variety of<br />
applications for the ideas.<br />
A remarkable and novel chapter on the ratchet and pawl as a heat eng<strong>in</strong>e attempts to l<strong>in</strong>k the<br />
otherwise quite dist<strong>in</strong>ct macroscopic and microscopic sets of arguments. <strong>The</strong> key to understand<strong>in</strong>g<br />
the nature of his approach is its selectivity. Figure 1 shows just how selective it is, as it<br />
<strong>in</strong>dicates how few of the topics discussed by others are picked out by Feynman.<br />
Choices amongst statistical arguments<br />
Any decision to offer a statistical approach h<strong>in</strong>ges on f<strong>in</strong>d<strong>in</strong>g some simple treatment of the<br />
statistics. Feynman f<strong>in</strong>esses the problem. Rather than do statistics, he treats a clearly statistical<br />
problem <strong>in</strong> a non-statistical style, choos<strong>in</strong>g to look at the exponential distribution with height<br />
of the density of an isothermal gas, from which he extracts the Boltzmann factor.<br />
<strong>The</strong> exponential atmosphere<br />
Feynman’s neat trick is to produce the simple argument that <strong>in</strong> an isothermal atmosphere <strong>in</strong><br />
equilibrium <strong>in</strong> a gravitational field, the density, and so the ratio of the numbers of molecules<br />
per unit volume at different heights, is given by<br />
n/n, = exp(-mgh/kT)<br />
He argues that there must be a difference of pressure across any small <strong>in</strong>terval dh, just sufficient<br />
to support the weight of the gas <strong>in</strong> that <strong>in</strong>terval, so that<br />
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