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VOLUME 73, NUMBER 7 PHYSICAL REVIEW LETTERS 15 AUGUST 1994

Statistical Distribution for Generalized Ideal Gas of Fractional-Statistics Particles

Yong-Shi Wu Department of Physics, University of Utah. Salt Lake City, Utah 84 J J2 (Recei ved 31 January 1994) We derive the occupation-number distribution in a generalized ideal gas of particles obeying fractional statistics, including mutual statistics, by adopting a state-counting definition. When there is no mutual statistics, the statistical distribution interpolates between and , and respects a fractional exclusion principle (except for bosons). Anyons in a strong magnetic field at low temperatures constitute such a physical system. Applications to the thermodynamic properties of excitations in the Laughlin quantum Hall fluid are discussed.

PACS numbers: 05.30.-{j, 05.70.Ce, 71.10.+x, 73.40.Hm Statistics is the distinctive property of a particle (or conditions and size of the condensed-matter region fixed. elementary excitation) that plays a fundamental role in The N -particle wave function, when the coordinates determining macroscopic or thermodynamic properties of of N - 1 particles and their species are held fixed, a quantum many-body system. In recent years, it has can be expanded in a basis of wave functions of the been recognized that particles with "fractional statistics" remaining particle. The crucial point is that in the intermediate between bosons and fermions can exist in presence of other particles, the number d; of available two-dimensional [1] or in one-dimensional [2,3] systems. single-particle states in this basis for a particle of species Most of the study has been done in the context of many­ i generally is not a constant, as given by G;; rather it body . There have been calculations may depend on the particle numbers {N;} of all species. of thermodynamic properties of certain systems [2,4-6] This happens, for example, when localized particle states with the help of exact solutions, but general formulation are nonorthogonal; as a result, the number of available of quantum (QSM) for ideal gas single-particle states changes as particles are added at with an occupation-number distribution that interpolates fixed size and boundary conditions. Haldane [3] defined between bosons and fermions is still lacking. the statistical interactions aij through the linear relation A single-particle quantum state can accommodate an arbitrary number of identical bosons, while no two identi­ (3) cal fermions can occupy one and the same quantum state (Pauli's exclusion principle). In QSM [7], this difference where {.:~Nj} is a set of allowed changes of the particle gives rise to different counting of many-body states, or numbers. In the same spirit, but more directly to the different statistical weight W. For bosons or fermions, purposes of QSM, we prefer defining the statistics by the number of quantum states of N identical particles oc­ counting [8] the number of many-body states at fixed {N;}, cupying a group of G states is, respectively, given by G. + N· - 1 - '. a··(N - 8.)J' (G + N - 1)! G! [ Il L..J IJ J IJ' W= . (4) Wb = N! (G _ 1)! or Wf = N! (G _ N)!' (I) n ; (N)'I' [G.I - 1 - L..J'. a··(N·IJ J - 8.)J'IJ'

A simple interpolation implying fractional exclusion is The parameters aij must be rational, in order that a W= [G+(N-1)(l-a)]! (2) thermodynamic limit can be achieved through a sequence N! [G - aN - (l - a)]! ' of systems with different sizes and particle numbers. We call aij for i *' j mutual statistics. We note that Eq. (4) i with a = 0 corresponding to bosons and a = 1 fermions. applies to the usual Bose or Fermi ideal gas with labeling Such an expression can be the starting point of QSM for single-particle energy levels and aij = a8;j (a = 0,1). intermediate statistics with 0 < a < 1. Let us first clarify So with an extension of the meaning of species, this its precise meaning in connection with "occupation of definition allows different species indices to refer to single-particle states," and justify it as a new definition particles of the same kind but with different quantum of quantum statistics, illa Haldane [3]. numbers [9]. Note there is no periodicity in so-defined Following Ref. [3], we consider the situations in which statistics, and it makes sense to consider the cases with the number G; of independent states of a single particle a > lor 2. (elementary excitation) of species i, confined to a finite As usual in QSM, we start with the ideal situations in region of matter, is finite and extensive, i.e., proportional which total energy (eigenvalue) is always a simple sum, to the size of the matter region in which the particle (5) exists. Now let us add more particles with the boundary

922 0031-9007/94/73 (7)/922(4)$06.00 © 1994 The American Physical Society VOLUME 73, NUMBER 7 PHYSICAL REVIEW LETTERS IS AUGUST 1994 with ei identified as the energy of a particle of species i. We call such a system a generalized [10] ideal gas Z = L W ({Ni})exp {LNi (/Li - ei) /kT}. (6) {N,l i if Eq. (4) also applies. Postponing the discussions about when Eqs. (4) and (5) are obeyed, let us first apply them to study QSM of generalized ideal gas. Following As usual, we expect that for very large Gi and N i , the the standard procedure [7], one may consider a grand summand has a very sharp peak around the set of most at temperature T and with chemical probable (or mean) particle numbers {Ni }. Using the potential /Li for species i. According to the fundamental Stirling formula In N! = N In (N / e), and introducing the principles of QSM, the grand partition function is given average "occupation number" defined by ni == NdGi, we by (with k the ) express In W as (with f3ij == aijGj/Gi)

~ G, {-n, In n, - (I -pun} (I - ~"'jn,) + [I + ~ (B'j - f3,j)n}{ + ~ (BU - ilu)n j]}

(7)

The most probable distribution of ni is determined by nj satisfies

a~i [In W + ~ Gini (/Li - ei) /kT ] = O. (8) and we have the statistical distribution It follows that I ni = , (IS) w(e(e, - JL)/kT) + a

where the function we?) satisfies the functional equation

(9) w(?)"[1 + w(?)]l-" = ? == e(e-JL)/kT. (16)

Note that we?) = ? - I for a = 0, and we?) = ? for a = l. Thus, Eq. (IS) recovers the familiar Bose and = 0 = (10) Fermi distributions, respectively, with a and a l. For semions with a = 1/2, Eq. (14) becomes a quadratic equation, which can be easily solved to give Therefore the most probable average occupation num­ = I bers ni (i 1,2, ... ) can be obtained by solving nj = . (17) .JI/4 + exp [2 (ei - f.L) /kT] L (8ij wj + (3ij) nj = I, (II) j For intermediate statistics 0 < a < I, it is not hard to se­ lect the solution w(?) ofEq. (16) that interpolates between with Wi determined by the functional equations (10). The bosonic and fermionic distributions. In particular, when? thermodynamic potential n = - kT In Z is given by is very large, we have we?) = ? and, neglecting a com­ l pared to we recover the Boltzmann distribution n == -PV = -kTLGln + ni - Lj{3ijnj (12) wen, i I I - Lj {3ijn j , (18) and the , S = (E - Li f.LiNi - n)/T, is at sufficiently low densities for any statistics. S , { ei - f.Li 1 + ni - L {3i jnj } - = L. Gi ni + In J. Furthermore, we note that? is always non-negative, so k i kT I - L {3ijnj is w; it follows from Eq. (IS) that J (13) Other thermodynamic functions follow straightforwardly. ni:S I/a. (I9) As usual, one can easily verify that the fluctuations, 2 2 (N/ - Ni )/Nj , of the occupation numbers are negligi­ This expresses the generalized exclusion principle for ble, which justifies the validity of the above approach. fractional statistics. In particular, at absolute zero, ? = 0 The simplest example is the ideal gas, i.e., identical if ei < /L, and? = +00 if ei > /L. From Eq. (16), we particles with no mutual statistics, for which we set ajj = have w = 0 and oc, respectively. Thus, we see that at T = a8ij and f.Li = /L. Then the average occupation number 0, for statistics a * 0, the average occupation numbers 923 VOLUME 73, NUMBER 7 PHYSICAL REVIEW LETTERS 15 AUGUST 1994 for single-particle states with continuous energy spectrum and (16) with only one energy e = !iwcl2, we have obey a step distribution like fermions: N P n == - ==- (26) O, if ei > E F , (20) G Po { ni = l/a, if ei < E F • where we?) is the positive solution of Eq. (16). Here P == The Fermi surface e = EF is determined by the require­ N /V is the areal density, and Po == I/Vo. Equation (26), L.e'<£f = aN. ment G, Below the Fermi surface, the av­ together with (16), determines the chemical potential Jl in erage occupation number is a for each single-particle 1/ terms of P / Po and T. Thermodynamic quantities can also state, in agreement with fractional exclusion. be expressed as functions of the ratio P / Po. In particular, One may be tempted to consider, in parallel to the usual the thermodynamic potential is Bose and Fermi ideal gas, the case with 2 V 1 + w V 1 + (1 - a) n !i k; G. = V(ak)2 = (21) n -kT-In-- -kT-ln . ei = 2m' , (21T)2' Vo w Vo 1 - an (27) say in two dimensions with V the area. Then treating The equation of state is momentum as continuous, one has the Fermi momentum PV = (!!.-)-l In 1 + (1 - a)p/po . (28) k~ = (41Ta)N/V. (22) NkT Po I - a(p/po) Moreover, at finite temperatures, by using (15) and (16), The pressure P is linear in T for fixed p. It diverges the sum L.i G;n; = N can be performed to give at the critical density Pc = (1/ a )Po, which corresponds 21Tfi2 2 to the complete filling of the LLL. The emergence !!:-. = a '!.- + In[1 - exp (_21T!i N)J. (23) of an incompressible state at filling fraction 1/ a is a kT mkT V mkT V consequence of the generalized exclusion principle (20) Using the identity derived by integration by parts, [17]. The magnetization per unit area is

x 1 - ani fOC ~A 2JlO 1 + (1 - a)p/po de; In ( ) = de;e;ni' (24) .J'~ = - /-toP + - In , (29) fo 1 + 1 - a ni 0 ,.\2 l-a(p/po) we have the statistics-independent relation PV = E. where Jlo = q!i/2mc is the Bohr magneton. Note the In the Boltzmann limit [exp(Jl/kT)« 1], we?) = first (de Haas-van Alphen) term is statistics independent. ? + a - I, At low temperatures, kT «!iwc, the second term can be neglected except for p very close to (l/a)po, where it PV = NkT [1 + (2a - I)N,.\2 /4V ] ' (25) gives rise to a nonvanishing, a-dependent susceptibility where ,.\ = J21T!i2 / mkT. So the "statistical interactions" X = kT-q- (-~) p/Po are attractive or repulsive depending on whether a < 1/2 21T!iC B (1 - ap/ po)[1 + (1 - a) p/ Po] . or a > 1/2. (30) Whether a given system satisfies the seemingly harm­ less conditions (5) or (21) together with (4) is highly The entropy per particle is also a dependent: nontrivial. It turns out [11] that statistical transmuta­ tion happens in 1D Bethe-ansatz solvable gas, so that ~ = k (1 - a + In [1 + (1 - a) both of these conditions apply if particles of different :0) :0 ] pseudomomenta can be viewed as belonging to differ­ ent species. On the other hand, while it was claimed [3] - k In :0 - k (:0 - a ) In (1 - a :0)' that the definition (4) for fractional statistics does not ap­ (31 ) ply to free anyons, i.e., Newtonian particles carrying flux tubes [12,13] in two spatial dimensions, anyons in a mag­ Equations (27), (28), and (29) have been derived in netic field are known to satisfy both (4) and (5) if all Ref. [6] from the known exact many-any on solutions in anyons are in the lowest Landau level (LLL) [14], as is the LLL. the case at very low temperatures. The Jastrow-type pref­ Vortexlike quasiparticle excitations in Laughlin's in­ actor na

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