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The Physical Basis of The Direction of Time (The Frontiers ...

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66 3 <strong>The</strong> <strong>The</strong>rmodynamical Arrow <strong>of</strong> <strong>Time</strong><br />

∫<br />

H gen [ρ(α)] := ρ(α)ln ρ(α) dα = ln p. (3.53)<br />

σ(α)<br />

<strong>The</strong> final form on the RHS is appropriate, since the mean probability p(α)<br />

for individual microscopic states and for given ρ(α) isthenp(α) =ρ(α)/σ(α).<br />

<strong>The</strong> entropy defined by −kH gen is also known as the relative entropy <strong>of</strong> ρ(α)<br />

with respect to the measure σ(α). <strong>The</strong> latter is <strong>of</strong>ten introduced ad hoc as<br />

part <strong>of</strong> a phenomenological description.<br />

Under the approximation w(α ′ ,α)=f(α)δ ′ (α − α ′ ) one now obtains the<br />

deterministic ‘drift’ limit <strong>of</strong> the master equation (3.51) – usually representing<br />

the first term <strong>of</strong> (3.44). It defines the first order <strong>of</strong> the Kramers–Moyal expansion<br />

for w(α, α ′ ), equivalent to an expansion <strong>of</strong> ρ(α ′ ,t) in terms <strong>of</strong> powers <strong>of</strong><br />

α ′ −α at α ′ = α. <strong>The</strong> second order, w(α ′ ,α)=f(α)δ ′ (α−α ′ )+g(α)δ ′′ (α−α ′ ),<br />

leads to the Fokker–Planck equation as the lowest non-trivial approximation<br />

that leads to an irreversible equation (see de Groot and Mazur 1962, Röpke<br />

1987). In this respect, it is analogous to the LAD equation as the lowest nontrivial<br />

order in the Taylor expansion <strong>of</strong> the Caldirola equation (2.31). A master<br />

equation is generally equivalent to a (stochastic) Langevin equation for individual<br />

macroscopic trajectories α(t) which may form a dynamical ensemble<br />

represented by ρ(α, t).<br />

In contrast to the Liouville equation (3.26), the master equation (3.48) or<br />

(3.36) cannot be unitary with respect to the inner product for probability distributions<br />

defined above (3.27). While total probability must be conserved by<br />

these equations, that <strong>of</strong> the individual trajectories cannot (see also Sect. 3.4).<br />

Information-reducing master equations describe an indeterministic evolution,<br />

which in general only determines an ever-increasing ensemble <strong>of</strong> different potential<br />

successors for each macroscopic state (such as a point in α-space). 7<br />

As discussed above, this macroscopic indeterminism is compatible with microscopic<br />

determinism if that information which is transformed from relevant<br />

7 <strong>The</strong> frequently used picture <strong>of</strong> a ‘fork’ in configuration space, characterizing a<br />

dynamical indeterminism, may be misleading, since it seems to imply unique<br />

predecessors. This would be wrong, as can be recognized, for example, in an<br />

equilibrium situation. In the case <strong>of</strong> a stochastic dynamical law that is defined on a<br />

finite set <strong>of</strong> states, a state must in general also have different possible predecessors,<br />

corresponding to an inverse fork. Inverse forks by themselves would represent<br />

a pure forward determinism (a ‘semigroup’, that may describe attractors). All<br />

these structures are meant to characterize the dynamical law. <strong>The</strong>y are neither<br />

properties <strong>of</strong> the (f)actual history (which is assumed to evolve along a definite<br />

trajectory regardless <strong>of</strong> the nature <strong>of</strong> the dynamical law), nor <strong>of</strong> an evolving<br />

ensemble that represents a specific state <strong>of</strong> knowledge.<br />

However, only dynamically unique predecessors may give rise to recordable<br />

histories (consisting <strong>of</strong> ‘facts’ that are redundantly documented). <strong>The</strong> historical<br />

nature <strong>of</strong> our world is thus based on a uniquely determined or even overdetermined<br />

macroscopic past – see also footnote 1 <strong>of</strong> Chap. 2, Fig. 3.8, and Sect. 3.5.<br />

A macroscopic history that was completely determined from its macroscopic past<br />

would be in conflict with the notion <strong>of</strong> an (apparent) free will.

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