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6 The H-theorem in κ-statistics: influence on the molecular chaos hypothesis 0 0 R. Silva∗† 2 Observat´orio Nacional, Rua Gal. Jos´e Cristino 77, 20921-400 Rio de Janeiro - RJ, Brasil n (Dated: February 2, 2008) a J We rediscuss recent derivations of kinetic equations based on the Kaniadakis’ entropy concept. Ourprimary objective hereisto derivea kineticalversion ofthesecond law of thermodynamycsin 4 suchaκ-framework. Tothisend,weassumeaslightmodificationofthemolecularchaoshypothesis. 2 For the Hκ-theorem, it is shown that the collisional equilibrium states (null entropy source term) ] aredescribedbyaκ-powerlawextensionoftheexponentialdistributionand,asshouldbeexpected, h all these results reduce to thestandard one in thelimit κ→0. c e PACSnumbers: 05.90.+m;05.20.-y;05.45.+b m - t I. INTRODUCTION The κ-statistic is defined by the κ-deformed functions, a given by t s t. Over the last few years, a great deal of attention exp (f)=( 1+κ2f2+κf)1/κ, (4) a has been paid to nonextensive statistic mechanics based κ m on the deviations of Boltzmann-Gibbs-Shannonentropic p - measure. Basically, in this extended framework, the key d point is to substitute the exponential behaviour of the fκ−f−κ n entropybyapower-lawone(see,e.q. [1]). Recently,sim- lnκ(f)= 2κ , (5) o ilar motivations also led at least to two new examples, c and [ namely, Abe [2, 3] and Kaniadakis entropies [4, 5]. In thislatterworks,byusingκ-exponentialandκ-logarithm exp (ln f)=ln (exp (f))=f. (6) 2 functions (see Eqs. (4) and (5)) and the kinetic interac- κ κ κ κ v 8 tion principle (KIP), Kaniadakis proposed a statistical Asonemaycheck,theabovefunctionsreducetothestan- 2 framework based on κ-entropy [4, 5] dard exponential and logarithm when κ → 0. In partic- 2 ular, this κ-framework leads to a class of one parameter 1 S (f)=− d3vf[a fκ+a f−κ+b ] (1) deformedstructureswithinterestingmathematicalprop- 1 κ Z κ −κ κ erties [6]. Recently, a connection with the generalized 5 Smoluchowski equation was investigated [7], and a fun- 0 where a and b are coefficients so that in limit κ → 0, κ κ damentaltest,i.e.,theso-calledLeschestabilitywasalso / t Eq. (1) reduces to the standard entropy Sκ=0. Expres- checked in the κ-framework [8]. More recently, it was a sion (1) is also the most general one that leads to the m shown that it is possible to obtain a consistent form for κ-framework. the entropy (linked with a two-parameter deformations - Previous works have already discussed some specific d oflogarithmfunction),whichgeneralizestheTsallis,Abe n choices for the constants aκ and bκ. For instance, for and Kaniadakis logarithm behaviours [9]. In the experi- o the pair [aκ = 1/2κ, bκ = 0], it is possible to write the mentalviewpoint,thereexistsomeevidencerelatedwith c Kaniadakis entropy as [3, 4] the κ-statistic, namely, cosmic rays flux, rain events in : v meteorology[6], quark-gluonplasma [10], kinetic models Xi Sκ =− d3vflnκf =−hlnκ(f)i, (2) describing a gas of interacting atoms and photons [11], Z fracture propagationphenomena [12], and income distri- r a bution [13], as well as constructfinancial models [14]. In whichhasaperfectanalogywiththestandardformalism. thetheoreticalfront,somestudiesonthecanonicalquan- The second and third choices are, respectively, [a = κ tization of a classical system has also been investigated 1/2κ(1+κ), b = 0] [4] and [a = 1/2κ(1+κ), b = κ κ κ [15]. −a −a ] [3] while the fourth one is given by [a = κ −κ κ In this letter, we aim at rediscussing the H-theorem Zκ/2κ(1+κ), b = 0] [4]. In particular, in this latter κ in the context of Kaniadakis entropy framework, Eq. choice, the κ-entropy is given by [4, 6] (3). However, instead of using the KIP introduced in zκ z−κ Ref. [6], we propose a different route to the κ-statistic S =− d3v f1+κ− f1−κ . (3) which follows similar arguments of Ref. [16]. In real- κ Z (cid:18)2κ(1+κ) 2κ(1−κ) (cid:19) ity, the main result is to obtain the equilibrium veloc- ity κ-distribution of a slight modification of the kinetic BoltzmannH-theorem,wherethecentralideafollowsby modifing the molecular chaos hypothesis and generaliza- ∗OnleaveofabsencefromUniversidadedoEstadodoRioGrande doNorte,59610-210, Mossoro´,RN,Brasil tion of the local entropy formula in accordance with a †Electronicaddress: [email protected],[email protected] κ-statistic. 2 II. THE MOLECULAR CHAOS HYPOTHESIS volume V. In BKT the state of a non-relativistic gas is characterized by the one-particle distribution func- As is widely known, the Boltzmann’s kinetic theory tion f(r,v,t), which is defined in such a way that (BKT) relies on two statistical ingredients, namely [17, f(r,v,t)d3rd3v gives at a time t, the number of parti- 18]: cles in the volume element d3rd3v around the particle position r and velocity v. Let us consider that distribu- • The local entropy which is expressed by Boltz- tion function is a solution of the κ-Boltzmann equation, mann’slogarithmicmeasure(Boltzmann’sconstant given by is an unity) ∂f ∂f F ∂f +v· + · =C (f), (10) ∂t ∂r m ∂v κ H[f] = − f(r,v,t) lnf(r,v,t)d3v. (7) where Cκ defines the κ-collisional term. In expression Z (10), the left-hand-side (LHS) is just the total time derivative of the distribution function, thus it is reason- • The hypothesis of molecular chaos able to consider that the unique possible modification (“Stosszahlansatz”), i.e., the two point corre- describing κ-statistic must be associated with the colli- lation function of the colliding particles can be sional term, which is clearly a hypothesis of work. Basi- factorized cally,C (f)maybecalculatedthroughthelawsofelastic κ collisions,where the standardassumptions arealso valid [17, 18]. f(r1,v1,r2,v2,t) = f(r1,v1,t)f(r2,v2,t). (8) As in the canonical H-theorem, our main goal here is toshowthatC (f)leadsto anonnegativeexpressionfor Thereissomecontroversyassociatedwiththe secondas- κ the time derivativeofthe κ-entropy,anddoesnotvanish sumption, Eq. (8). In particular, Burbury [19], was the unless the distribution function assumes the equilibrium first to point out that this hypothesis provides the fun- form for a κ-distribution which has been recently pro- damental role within the BKT. Physically, the equation posed [6]. Here, we define (8) represents that colliding molecules are uncorrelated, i.e., the velocities and positions of pairs of molecules are s2 statistically independents. The irreversibility associated Cκ(f)= |V·e|Rκdωd3v1, (11) 2 Z withtheBoltzmann’sequationcanbetracedbacktothis assumption. Indeed,asthemoleculeswhichhasbeenas- whered3v1 isanarbitraryvolumeelementinthevelocity sumed to be uncorrelated before a collision, become cor- space, V denotes the relative velocity before collision, related after the collision, this clearly represents a time V = v1 −v, e denotes an arbitrary unit vector, dω is asymmetric hypothesis [20]. In particular, this hypothe- an elementary solid angle such that s2dω is the area of sismaynotalwaysbe validforrealgases(see[21,22]for the “collision cylinder” (for details see Refs. [17, 18]), details). finallyR (f,f′)isadiferenceoftwocorrelationfunctions κ In this investigation, we introduce a consistent gener- (just before and after collision). In this approach, such alizationofthis hypothesis,expression(8), within the κ- expression is assumed to satisfy a κ-generalized form of statistic proposed by Kaniadakis. We remark that equa- molecular chaos hypothesis, which is given by tion (8) implies that the logarithm of the joint distri- bution f(r1,v1,r2,v2,t) describing coliding molecules is Rκ =expκ(lnκz′f′+lnκz′1f1′) given by lnf(r1,v1,r2,v2,t) = lnf(r1,v1,t)+lnf(r2,v2,t) (9) −expκ(lnκzf +lnκz1f1), (12) where each term involve only the marginal distribution whereprimesrefertothedistributionfunctionaftercolli- associated with one of the colliding molecules. The new sion,z,z′arearbitraryconstantandexp (f),ln (f),are κ κ hypothesis assumed here is to consider that a power of defined by Eqs. (2) and (3). Note that κ→0 the above the joint distribution (instead of the logarithm) be equal expression reduces to R0 = (z′f′)(z1′f′1) − (zf)(z1f1), to the sumoftwo terms,eachonedepending onjust one whereisonestandardtothemolecularchaoshypothesis. of the coliding molecules. Considering the κ-logarithm In the present framework, we adopt Kaniadakis for- function,theconditionabovecanbeformulatedinaway mula for local entropy that extend the standard hypothesis, Eq. (8). zκ z−κ H =− d3v f1+κ− f1−κ . κ Z (cid:18)2κ(1+κ) 2κ(1−κ) (cid:19) III. H-THEOREM AND κ-STATISTICS (13) Here, in order to obtain the source term, we need the partial time derivative of H Let us now introduce a spatially homogeneous gas of κ N hard-sphere particles of mass m and diameter s, un- ∂H ∂f κ =− d3vln fz , (14) der the action of an external force F, and enclosed in a ∂t Z κ ∂t 3 and combining with the κ-Boltzmann equation (10) and Now, in order to make the H-theorem and the κ- (11), one may rewrite the expression in the form of a statistic compatible,we need to recoverthe relatedequi- balance equation librium distribution previously obtained by an extrem- izationofκ-entropyandKIP[6]. TheH -theoremstates κ ∂H κ +∇·S =G (r,t), (15) that Gκ = 0 is a necessary and sufficient condition for k κ ∂t equilibrium. Since the integrandof (18) cannot be nega- tive, this occur if and only if wherethe κ-entropyfluxvectorrelatedtoH isgivenby κ lnκz′f′+lnκz1′f1′ =lnκzf +lnκz1f1 (22) zκ z−κ Sκ =− d3vv f1+κ− f1−κ , Therefore,theabovesumofκ-logarithmsremainscon- Z (cid:18)2κ(1+κ) 2κ(1−κ) (cid:19) stant during a collision, or equivalently, it is a summa- (16) tional invariant. Indeed, the unique quantities satisfying and the source term reads (18) are the particle masses, and the expressionsfor mo- −s2 mentumandenergyconservationlaws,whichleadto the Gκ = 2 Z |V·e|lnκfz Rκdωd3v1d3v. (17) following expression At this point, it is convenient to rewrite Gκ in a more lnκzf =ao+a1.v+a2v2, (23) symmetrical form by using some elementary symmetry operations which also take into account the inverse col- where ao and a2 are constants and a1 is an arbitrary lisions. First we notice that by interchanging v and v1 constantvector. Byintroducingthe barycentricvelocity, the value of the integral is preserved. This happens be- u, we may rewrite (23) as cause the magnitude of the relative velocity vector and 2 the scattering cross section are invariants [18]. In addi- ln zf =α−γ(v−u) , (24) κ tion, the value of G is not altered if we integrate with κ respect to the variables v′ and v′. Actually, although with a different set of constants. Thus, we obtain a κ- 1 changing the sign of R in this step (inverse collision), distribution κ the quantity d3vd3v1 is also a collisional invariant [18]. 1 As one may check, such considerations imply that the f = exp [α−γ(v−u)2], (25) z κ κ-entropy source term can be written as whereγ andumaybefunctionsofthetemperature. The s2 G (r,t)= |V·e|(ln z′f′ +ln z′f′− expressionaboveisthe generalformofthe κ-Maxwellian κ 8 Z κ 1 1 κ distribution function. −lnκz1f1−lnκzf)[expκ(lnκz′f′+lnκz′1f1′)− IV. FINAL REMARKS −expκ(lnκzf +lnκz1f1)]dωd3v1d3v. (18) Summing up, we have discussed a κ-generalization of Boltzmann’s kinetic equation along the lines defined by Notethattheintegrandin(18)isnevernegative,because κ-statistic. The main results follow from a slight modifi- the expressions cationofthemainstatisticalhypothesisunderlyingBoltz- mann’s approach: (lnκz′f′+lnκz1′f1′ −lnκzf −lnκz1f1) (19) 1. The κ-statistic has been explicitly introduced and through a new functional formula for the local en- expκ(lnκz′f′+lnκz1′f′1)−expκ(lnκzf +lnκz1f1)(20) tropy; 2. A nonfactorizable expression for the molecular alwayshavethesamesigns. Therefore,forvaluesofκon chaos hypothesis has been adopted. the interval [−1;1], we obtain ∂H Both ingredients are shown to be consistent with the κ +∇·Sκ =Gκ ≥0, (21) standard laws describing the microscopic dynamics, and ∂t reduce to the familiar Boltzmann assumptions in the which is the mathematical expression for the Hκ- limit (κ=0). theorem. Thisinequalitystatesthattheκ-entropysource Acknowledgments: The author is grateful to J. S. Al- must be positive or zero, thereby furnishing a kinetic caniz,I.QueirozandJ.A.S.Limaforhelpfuldiscussions. derivation of the second law of thermodynamics in the This work was supported by Conselho Nacional de De- κ-ststistic. senvolvimento Cient´ifico e Tecnol´ogico - CNPq (Brasil). 4 [1] C. Tsallis, J. Stat. Phys. 52, 479 (1988); S. R. A. [12] M.Cravero,G.Labichino,G.Kaniadakis,E.Miraldiand Salinas and C. Tsallis (Eds.), Braz. J. Phys. (spe- A. M. Scarfone, Physica A 340, 410 (2004) cial number) 29 (1999); S. Abe and Y. Okamoto [13] A. Dragulescu, cond-mat/0307341 (Eds.), Nonextensive Statistical Mechanics and Appli- [14] D. Rajaonarison, D. Bolduc and H. Jayet, Econ. Lett. cations, Springer, Heidelberg (2001); M. Gell-Mann 86, 13 (2005) and C. Tsallis (Eds.), Nonextensive Entropy - Inter- [15] A. M. Scarfone, Phys. Rev.E 71, 051103 (2005) disciplinary Applications, Oxford University Press, New [16] R. Silva, A. R. Plastino and J. A. S. Lima, Phys. Lett. York (2004). An updated bibliography can be found in A 249, 401 (1998); J. A. S. Lima, R. Silva and A. R. http://tsallis.cat.cbpf.br/biblio.htm Plastino, Phys.Rev. Lett. 86, 2938 (2001) [2] S.Abe, Phys.Lett. A 224, 326 (1997) [17] C. J. Thompson, Mathematical Statistical Mechanics, [3] S. Abe, G. Kaniadakis, and A. M. Scarfone, J. Phys. A: Princeton UniversityPress (1979) Math. Gen. 37, 10513 (2004) [18] A. Sommerfeld, Thermodynamics and Statistical Me- [4] G. Kaniadakis, Physica A 296, 405 (2001) chanics, Lectures on Theorethical Physics, Vol. V, Aca- [5] G. Kaniadakis, Phys.Rev.E 66 056125 (2002) demic Press, New York (1993) [6] G. Kaniadakis, Phys. Lett. A 288, 283 (2001); G. Kani- [19] S.H. Burbury,Nature, 51, 78 (1894). adakis and A. M. Scarfone, Physica A, 305, 69 (2002); [20] H.D. Zeh, The Physical Basis of The Direction of Time, G.kaniadakis,P.QuaritiandA.M.Scarfone,PhysicaA, Springer-Verlag, Berlin-Heidelberg (1992) 305, 76 (2002) [21] Ludwig Boltzmann, Lectures in Gas Theory, Berkeley:, [7] P.H. Chavanis, P. Laurencot and M. Lemou, Physica A University of California Press (1964) 341, 145 (2004) [22] S.G.Brush,Statistical PhysicsandtheAtomicTheoryof [8] G. Kaniadakis and A.M. Scarfone, Physica A, 340, 102 Matter, fromBoyle andNewton toLandau andOnsager, (2004); G. Kaniadakis, M. Lissia and A. M. Scarfone, Princeton UniversityPress, Princeton (1983) Physica A 340, 41 (2004) [23] I. V. Karlin, M. Grmela, and A. N. Gorban, Phys. Rev [9] G.Kaniadakis,M.LissiaandA.M.Scarfone,Phys.Rev. E 65, 036128 (2002) E 71, 046128 (2005) [24] A.Lavagno,G.Kaniadakis,M.Rego-Monteiro,P.Quar- [10] A.M.Teweldeberhan,H.G.MillerandR.Tegen,Int.J. iti and C. Tsallis, Asthop. Lett. and Comm., 35, 449 Mod. Phys. E 12, 669 (2003) (1998) [11] A. Rossani and A. M. Scarfone, J. Phys. A: Math. 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