Zwanzig projection operator

The Zwanzig projection operator is a mathematical device used in statistical mechanics.[1] This projection operator acts in the linear space of phase space functions and projects onto the linear subspace of "slow" phase space functions. It was introduced by Robert Zwanzig to derive a generic master equation. It is mostly used in this or similar context in a formal way to derive equations of motion for some "slow" collective variables.[2]

Slow variables and scalar product edit

The Zwanzig projection operator operates on functions in the  -dimensional phase space   of   point particles with coordinates   and momenta  . A special subset of these functions is an enumerable set of "slow variables"  . Candidates for some of these variables might be the long-wavelength Fourier components   of the mass density and the long-wavelength Fourier components   of the momentum density with the wave vector   identified with  . The Zwanzig projection operator relies on these functions but does not tell how to find the slow variables of a given Hamiltonian  .

A scalar product[3] between two arbitrary phase space functions   and   is defined by the equilibrium correlation

 

where

 

denotes the microcanonical equilibrium distribution. "Fast" variables, by definition, are orthogonal to all functions   of   under this scalar product. This definition states that fluctuations of fast and slow variables are uncorrelated, and according to the ergodic hypothesis this also is true for time averages. If a generic function   is correlated with some slow variables, then one may subtract functions of slow variables until there remains the uncorrelated fast part of  . The product of a slow and a fast variable is a fast variable.

The projection operator edit

Consider the continuous set of functions

 
with   constant. Any phase space function   depending on   only through   is a function of the  , namely
 

A generic phase space function   decomposes according to

 

where   is the fast part of  . To get an expression for the slow part   of   take the scalar product with the slow function  ,

 

This gives an expression for  , and thus for the operator   projecting an arbitrary function   to its "slow" part depending on   only through  ,

 

This expression agrees with the expression given by Zwanzig,[1] except that Zwanzig subsumes   in the slow variables. The Zwanzig projection operator fulfills   and  . The fast part of   is  . Functions of slow variables and in particular products of slow variables are slow variables. The space of slow variables thus is an algebra. The algebra in general is not closed under the Poisson bracket, including the Poisson bracket with the Hamiltonian.

Connection with Liouville and Master equation edit

The ultimate justification for the definition of   as given above is that it allows to derive a master equation for the time dependent probability distribution   of the slow variables (or Langevin equations for the slow variables themselves).

To sketch the typical steps, let   denote the time-dependent probability distribution in phase space. The phase space density   (as well as  ) is a solution of the Liouville equation

 

The crucial step then is to write  ,   and to project the Liouville equation onto the slow and the fast subspace,[1]

 
 

Solving the second equation for   and inserting   into the first equation gives a closed equation for   (see Nakajima–Zwanzig equation). The latter equation finally gives an equation for   where   denotes the equilibrium distribution of the slow variables.

Nonlinear Langevin equations edit

The starting point for the standard derivation of a Langevin equation is the identity  , where   projects onto the fast subspace. Consider discrete small time steps   with evolution operator  , where   is the Liouville operator. The goal is to express   in terms of   and  . The motivation is that   is a functional of slow variables and that   generates expressions which are fast variables at every time step. The expectation is that fast variables isolated in this way can be represented by some model data, for instance by a Gaussian white noise. The decomposition is achieved by multiplying   from the left with  , except for the last term, which is multiplied with  . Iteration gives

 

The last line can also be proved by induction. Assuming   and performing the limit   directly leads to the operator identity of Kawasaki[2]

 

A generic Langevin equation is obtained by applying this equation to the time derivative of a slow variable  ,  ,

 

Here   is the fluctuating force (it only depends on fast variables). Mode coupling term   and damping term   are functionals of   and   and can be simplified considerably.[1][2][4]

Discrete set of functions, relation to the Mori projection operator edit

Instead of expanding the slow part of   in the continuous set   of functions one also might use some enumerable set of functions  . If these functions constitute a complete orthonormal function set then the projection operator simply reads

 

A special choice for   are orthonormalized linear combinations of the slow variables  . This leads to the Mori projection operator.[3] However, the set of linear functions is not complete, and the orthogonal variables are not fast or random if nonlinearity in   comes into play.

See also edit

References edit

  1. ^ a b c d Zwanzig, Robert (1961). "Memory Effects in Irreversible Thermodynamics". Phys. Rev. 124 (4): 983–992. Bibcode:1961PhRv..124..983Z. doi:10.1103/physrev.124.983.
  2. ^ a b c Kawasaki, K. (1973). "Simple derivations of generalized linear and nonlinear Langevin equations". J. Phys. A: Math. Nucl. Gen. 6 (9): 1289–1295. Bibcode:1973JPhA....6.1289K. doi:10.1088/0305-4470/6/9/004.
  3. ^ a b Mori, H. (1965). "Transport, Collective Motion, and Brownian Motion". Prog. Theor. Phys. 33 (3): 423–455. Bibcode:1965PThPh..33..423M. doi:10.1143/ptp.33.423.
  4. ^ Gunton, J.D. (1979). "Mode coupling theory in relation to the dynamical renormalization group method". Dynamical Critical Phenomena and Related Topics. Lecture Notes in Physics. Vol. 104. pp. 1–24. Bibcode:1979LNP...104....1G. doi:10.1007/3-540-09523-3_1. ISBN 978-3-540-09523-1.