Institute of Experimental Physics, University of Vienna
The teaching of Statistical Physics in the basic physics course is both indispensible and impossible: indispensible because Thermodynamics
cries for an explanation, and impossible since students have insufficient mathematical training at this point.
To resolve this dilemma we make use of two important developments of the last decades: microscopic simulation and deterministic chaos.
Specifically, we do in-class live simulations of model systems, and we invoke intuitive geometrical arguments to explore Gibbs'
phase space.
PCs have recently become powerful enough to do a nontrivial simulation within 1-2 minutes, which is the attention span available
in a lecture setting. Thus we are now in position to use the PC together with a data projector in the same way as any other
setup for a lecture-hall experiment. In addition, using the Java technology we can make the simulation program available to students
for exercises and projects.
Chaos theory has yielded a result which is of utmost practical importance in didactics: chaos can be found in systems with no more
than two degrees of freedom. This means that we can actually d r a w the phase space and the energy surface (line, rather) of
such a system and demonstrate that the microstates are indeed equally distributed. The`assumption' of equal a priori probability on the
energy surface has thus become an experimental, demonstrable fact.
On the basis of this evidence we may now go on to more degrees of freedom. Studying hard discs systems with increasing numbers of
particles we may invite students to explore the simple but surprising properties of multidimensional space. Since hard bodies have a
hyperspherical energy surface, we have to deal only with very simple objects in phase space. In particular, we may predict and verify the
distribution of one velocity component in a system of 1, 2, or more hard discs and hard balls. Very soon this distribution approaches a
Gaussian (see Figure) and thus yields the Maxwell-Boltzmann distribution for the modulus of the particle velocity.
Having understood phase space and energy surfaces, we can go on to make the all-important transition from statistics to
thermodynamics. The vehicle for this traversal is S, the entropy. We make the tentative assumption that S is given by the log of the
phase space volume of the system. Next we demonstrate that this quantity has indeed the constitutive properties of the entropy:
additivity and the fact that S governs the energy transfer between two systems in contact: dE/dS (temperature) must be
equal in both systems. While this argument is rather too abstract for second-year students, it can be visualised
easily by letting a given amount of energy be divided up between two systems in all possible proportions. It becomes
evident that the most probable situation, having the largest phase space volume, is just the one given by the equal
temperature law.
After these discoveries we are in a position to assemble all the basic facts of Statistical Physics commonly encountered
in textbooks: ensembles, partition functions, free energies, quantum statistics, basic kinetic theory.
A short writeup of the present paper, including four sample Java programs, may be accessed via
http://www.ap.univie.ac.at/users/ves/grc2000/bx.
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