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# Specification of State of Many-Particle System

Let us first consider how we might specify the state of a many-particle system. Consider the simplest possible dynamical system, which consists of a single spinless particle moving classically in one dimension. Assuming that we know the particle's equation of motion, the state of the system is fully specified once we simultaneously measure the particle's displacement, , and momentum, . In principle, if we know and then we can calculate the state of the system at all subsequent times using the equation of motion. In practice, it is impossible to specify and exactly, because there is always an intrinsic error in any experimental measurement.

Consider the time evolution of and . This can be visualized by plotting the point ( , ) in the - plane. This plane is generally known as phase-space. In general, as time progresses, the point ( , ) will trace out some very complicated pattern in phase-space. Suppose that we divide phase-space into rectangular cells of uniform dimensions and . Here, is the intrinsic error in the position measurement, and the intrinsic error in the momentum measurement. The area of each cell is (3.1)

where is a small constant having the dimensions of angular momentum. The coordinates and can now be conveniently specified by indicating the cell in phase-space into which they plot at any given time. This procedure automatically ensures that we do not attempt to specify and to an accuracy greater than our experimental error, which would clearly be pointless.

Let us now consider a single spinless particle moving in three dimensions. In order to specify the state of the system, we now need to know three - pairs: that is, - , - , and - . Incidentally, the number of - pairs needed to specify the state of the system is usually called the number of degrees of freedom of the system. (See Section B.1.) Thus, a single particle moving in one dimension constitutes a one degree of freedom system, whereas a single particle moving in three dimensions constitutes a three degree of freedom system.

Consider the time evolution of and , where , et cetera. This can be visualized by plotting the point ( , ) in the six-dimensional - phase-space. Suppose that we divide the - plane into rectangular cells of uniform dimensions and , and do likewise for the - and - planes. Here, and are again the intrinsic errors in our measurements of position and momentum, respectively. This is equivalent to dividing phase-space up into regular six-dimensional cells of volume . The coordinates and can now be conveniently specified by indicating the cell in phase-space into which they plot at any given time. Again, this procedure automatically ensures that we do not attempt to specify and to an accuracy greater than our experimental error.

Finally, let us consider a system consisting of spinless particles moving classically in three dimensions. In order to specify the state of the system, we need to specify a large number of - pairs. The requisite number is simply the number of degrees of freedom, . For the present case, , because each particle needs three - pairs. Thus, phase-space (i.e., the space of all the - pairs) now possesses dimensions. Consider a particular pair of conjugate (see Section B.4) phase-space coordinates, and . As before, we divide the - plane into rectangular cells of uniform dimensions and . This is equivalent to dividing phase-space into regular dimensional cells of volume . The state of the system is specified by indicating which cell it occupies in phase-space at any given time.

In principle, we can specify the state of the system to arbitrary accuracy, by taking the limit . In reality, we know from Heisenberg's uncertainty principle (see Section C.8) that it is impossible to simultaneously measure a coordinate, , and its conjugate momentum, , to greater accuracy than . Here, is Planck's constant divided by . This implies that (3.2)

In other words, the uncertainty principle sets a lower limit on how finely we can chop up classical phase-space.

In quantum mechanics, we can specify the state of the system by giving its wavefunction at time , (3.3)

where is the number of translational degrees of freedom, and the number of internal (e.g., spin) degrees of freedom. (See Appendix C.) For instance, if the system consists of spin-one-half particles then there will be translational degrees of freedom, and spin degrees of freedom (because the spin of each particle can either be directed up or down along the -axis). Alternatively, if the system is in a stationary state (i.e., an eigenstate of the Hamiltonian) then we can just specify quantum numbers. (See Sections C.9 and C.10.) Either way, the future time evolution of the wavefunction is fully determined by Schrödinger's equation. In reality, this approach is not practical because the Hamiltonian of the system is only known approximately. Typically, we are dealing with a system consisting of many weakly-interacting particles. We usually know the Hamiltonian for completely non-interacting particles, but the component of the Hamiltonian associated with particle interactions is either impossibly complicated, or not very well known. We can define approximate stationary eigenstates using the Hamiltonian for non-interacting particles. The state of the system is then specified by the quantum numbers identifying these eigenstates. In the absence of particle interactions, if the system starts off in a stationary state then it stays in that state for ever, so its quantum numbers never change. The interactions allow the system to make transitions between different stationary'' states, causing its quantum numbers to change in time.   Next: Principle of Equal A Up: Statistical Mechanics Previous: Introduction
Richard Fitzpatrick 2016-01-25