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5. Formulation of Quantum Statistics

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1 5. Formulation of Quantum Statistics
Quantum Mechanical Ensemble Theory: The Density Matrix Statistics of the Various Ensembles Examples Systems Composed of Indistinguishable Particles The Density Matrix & the Partition Function of a System of Free Particles

2 Statistics Particle type Math Object
Classical Distinguishable Phase space density Quantum Indistinguishable Density matrix Advantage of using density matrix : Quantum & ensemble averaging are combined into one averaging.

3 Classical Statistical Mechanics
(Probability) density function  ( p,q,t ) : Caution: Some authors, e.g., Landau-Lifshitz, use a normalized version of  . Liouville’s theorem : Microcanonical ensemble : Canonical ensemble : Grand canonical ensemble :

4 Quantum Statistical Mechanics (To be Proved)
Ensemble = phase space Classical mechanics : Ensemble = Hilbert space Quantum mechanics : PE = projection operator onto the N-D subspace of states with energy E. Microcanonical : Canonical : Grand canonical :

5 Pure State Density Operator
Orthonormal basis { | n  } is complete : Expectation value of f : Density operator for |   :

6 r-Representation f is a 1-particle operator 

7 Mixed State Density Operator
Averaged value of f : Orthonormal basis { | n  } is complete : Density operator : Skip to ensembles Ex: Derive the quantum Liouville eq.

8 5.1. Quantum Mechanical Ensemble Theory: The Density Matrix
Consider ensemble of N identical systems labelled by k = 1, 2,..., N. Each system is described by i = 1,2,..., N  k runs through all independent solutions of this Schrodinger eq. Let be the wave function of the kth system in the ensemble. Let be a set of complete orthonormal basis that spans the Hilbert space of H & satisfies the relevant B.C.s. with

9 where H can be t-dep  k

10 Density Operator Density operator :
pk = weighting (or probability) factor with Matrix elements : n or  d ~ quantum averaging  ens ~ k ~ ensemble averaging

11 where H can be t-dep

12 Equilibrium Ensemble System in equilibrium  ensemble stationary :
i.e. and Energy representation : System in equilibrium  In a general basis ,  is hermitian  detailed balance

13 Expectation Values Expectation value of a physical quantity G :
( Quantum + ensemble av. ) Assuming k normalized, i.e., i.e. k normalized :

14 5.2. Statistics of the Various Ensembles
Microcanonical ensemble : Fixed N, V, E or ( quantum statistics: no Gibbs’ paradox ) ( N, V, E;  ) = # of accessible microstates Equal a priori probabilities postulate  Energy representation: i.e.

15 Pure State Only 1 state  p is accessible   3rd law  
Energy representation : Thus i.e. idempotent (  is a projector ) In another representation with basis { m } so that ,  normalized

16 Mixed State Multiple states are accessible, i.e.  > 1.
Any representation : = set of accessible state indices Let K be the subspace spanned by the accessible  k ’s. Consider any orthonormal basis {n } such that Since { k } is a basis of K, its completeness means (  is diagonal w.r.t. {n } )

17 Let  k = ensemble member index  So that Postulate of a priori random phases

18 Canonical Ensemble E-representation : i.e.
Canonical ensemble : Fixed N, V, T. By definition

19 Grand Canonical Ensemble
Grand canonical ensemble : Fixed , V, T Er, s = Er (Ns ) = E of r th state of Ns p’cle sys

20 5.3. Examples An Electron in a Magnetic Field signed
Single e with spin & magnetic moment Pauli matrices : A diagonal  agrees with §

21 A Free Particle in a Box Free particle of mass m in a cubical box of sides L. with Periodic B.C : with

22 ( r - representation ) with ( see next page )

23

24  is symmetric Location uncertainty : Particle density at r :

25 Alternatively Uising & integrate by parts twice :

26 A Simple Harmonic Oscillator
n = 0,1,2,... Hermite polynomials : Rodrigues’ formula

27 is real Kubo, “Stat Mech.”, p.175 Mathematica

28 Probability density :  q is a Gaussian with dispersion ( r.m.s. deviation ) :

29 Classical limit : (purely thermal) Quantum limit : (non-thermal) = Probability density of ground state

30

31 5.4. Systems Composed of Indistinguishable Particles
N non-interacting particles subject to the same 1-particle hamiltonian h. i = label of the eigenstate assumed by the i th particle. Let n = # of particles occupying the  th eigenstate. L( , j ) = label of the j th particle that occupies the  th eigenstate.

32 Note: [ ... ] = 1 if n = 0. Let P denote a permutation of the particle labels :

33 Distinguishable particles :
permutations within the same  counted as the same. permutations across different ’s counted as distinct.  # of distinct microstates is Indistinguishable particles : Boltzmannian ( distinguishable p’cles)

34 Indistinguishable Particles
Particles indistinguishable  Physical properties unchanged under particle exchange i.e.

35 Anti-symmetric : Pauli’s exclusiion principle i.e. Fermi-Dirac statistics Symmetric : Bose-Einstein statistics

36 5.5. The Density Matrix & the Partition Function of a System of Free Particles
N non-interacting, indistinguishable particles : Let i stands for ri , & i  for ri . e.g., Goal: To write or

37 Non-interacting particles 
Periodic B.C.  Bosons Fermions Mathematica

38 Consider the N ! permutations among { ki } associated with a given K.
 E is unchanged nk > 1 cases neglected (measure 0)

39 arbitrary P  P  = I 2-p'cle

40 from § 5.3 = thermal ( de Broglie ) wavelength

41 mean inter-particle distance = n = particle density
Let with Mathematica mean inter-particle distance = n = particle density

42 Resolution of problems in classical statistics:
Gibbs correction factor ( 1 / N! ). Phase space volume per state Classical limit : Non-classical systems are said to be degenerate.  n 3 = degeneracy discriminant ( no spatial correlation ) Classical limit

43 Exchange Correlation Let N = 2 :

44 Classical limit

45 Statistical Potential
Mathematica


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