=Paper= {{Paper |id=Vol-2300/Paper19 |storemode=property |title=Generalized Transport Equation with Fractality of Space-Time. Zubarev’s NSO Method |pdfUrl=https://ceur-ws.org/Vol-2300/Paper19.pdf |volume=Vol-2300 |authors=Petro Kostrobij,Bogdan Markovych,Olexandra Viznovych,Mykhailo Tokarchuk |dblpUrl=https://dblp.org/rec/conf/acit4/KostrobijMVT18 }} ==Generalized Transport Equation with Fractality of Space-Time. Zubarev’s NSO Method== https://ceur-ws.org/Vol-2300/Paper19.pdf
                                                                    75


            Generalized Transport Equation with Fractality
               of Space-Time. Zubarev’s NSO Method
    Petro Kostrobij1, Bogdan Markovych1, Olexandra Viznovych1, Mykhailo Tokarchuk1,2
         1. Lviv Polytechnic National University, 12 S. Bandera str., 79013, Lviv, Ukraine, email: bohdan.m.markovych@lpnu.ua
    2. Institute for Condensed Matter Physics of the National Academy of Sciences of Ukraine, 1 Svientsitskii str., 79011, Lviv, Ukraine


                                                                                                                                            
   Abstract: We presented a general approach for obtai-                      ∂
                                                                                                               (  
                                                                                                                              )               (               )
                                                                                                N                        N

ning the generalized transport equations with fractional                       ρ ( x N ; t ) + ∑Drα ρ ( x N ; t )v j + ∑Dαp ρ ( x N ; t ) F j = 0, (1)
                                                                            ∂t                 j =1
                                                                                                           j
                                                                                                                        j =1
                                                                                                                                          j

derivatives by using the Liouville equation with fractional                                                        
derivatives for a system of classical particles and the Zu-              where x = x1 , , x N , x j = {r j , p j } are dimensionless gene-
                                                                                    N

barev nonequilibrium statistical operator (NSO) method                                               
                                                                         ralized coordinates, r j = (r j1 , , r jm ) , and generalized mo-
within Renyi statistics. Generalized Cattaneo-type diffu-                             
sion equations with taking into account fractality of spa-               mentum, p j = ( p j1 , , p jm ) , [14] of j th particle in the pha-
ce-time are obtained.                                                    se space with a fractional differential volume element [13],
   Keywords: fractional derivative, diffusion equation.                  [15] d αV = d α x1  d α x N . Here, m = Mr0 ( p0t0 ) , M is the
                      I. INTRODUCTION                                    mass of particle, r0 is a characteristic scale in the configura-
   The fractional derivatives and integrals [1]–[4] are widely           tion space, p0 is a characteristic momentum, and t0 is a cha-
used to study anomalous diffusion in porous media, in disor-             racteristic time, d α is a fractional differential [15],
dered systems, in plasma physics, in turbulent, kinetic, and                                                       2N
reaction-diffusion processes, etc. [5], [6]. In Ref. [5], [6], we
discussed various approaches to obtaining the transport equ-
                                                                                                   d α f ( x) =    ∑D f ( x)(dx ) ,
                                                                                                                   j =1
                                                                                                                          α
                                                                                                                          xj                  j
                                                                                                                                                  α


ations with fractional derivatives. It is important to note that,        where
for the first time, in Refs. [7]–[10], Nigmatullin received dif-                                             1         x  f (n) ( z)
fusion equation with the fractional time derivatives for the
mean spin density [7], the mean polarization [8], and the
                                                                                              Dxα f ( x) =                        ∫
                                                                                                         Γ(n − α ) 0 ( x − z )α +1− n
                                                                                                                                      dz     (2)

charge carrier concentration [9]. In Ref. [10], justification of          is the Caputo fractional derivative, [1], [2], [16], [17]
equations with fractional derivatives is given, and the time ir-          n − 1 < α < n , f ( n ) ( z ) = d n f ( z ) dz n with the properties
reversible Liouville equation with the fractional time derivati-                                                       
ve is provided. In our recent work [5], by using NSO method               Dxαj 1 = 0 and Dxαj xl = 0 , ( j ≠ l ) . v j are the fields of veloci-
                                                                                                                                        
[11], [12] and the maximum entropy principle for the Renyi               ty, F j is the force field acting on j th particle. If F j does not
entropy, we obtained the generalized (non-Markovian) diffu-                                                               
sion equation with fractional derivatives. The use of the Liou-          depend on p j , v j does not depend on r j , and the Helmholtz
ville equation with fractional derivatives proposed by Tarasov           conditions, we get the Liouville equation in the form
in Refs. [13], [14] is an important and fundamental step for                                   ∂
                                                                                                 ρ ( x N ; t ) + iLα ρ ( x N ; t ) = 0,                    (3)
obtaining this equation. By using NSO method and the maxi-                                    ∂t
mum entropy principle for the Renyi entropy, we found a so-              where iLα is the Liouville operator with the fractional deri-
lution of the Liouville equation with fractional derivatives at
                                                                         vatives,
a selected set of observed variables. We chose nonequilibri-
                                                                                                       [                           
                                                                                                                                                          ]
                                                                                              N
um average values of particle density as a parameter of re-               iLα ρ ( x N ; t ) = ∑ Dαp H (r , p ) Drα − Drα H (r , p ) Dαp ρ ( x N ; t ). (4)
duced description, and then we received the generalized (non-                                   j =1
                                                                                                           j              j           j               j


Markovian) diffusion equation with fractional derivatives. In                             
                                                                         where H (r , p ) is a Hamiltonian of a system with fractional
the next section by using Ref. [5], new non-Markovian diffu-
sion equations for particles in a spatially heterogeneous envi-          derivatives [13]. A solution of the Liouville equation (3) will
ronment with fractal structure are obtained. Different models            be found with Zubarev`s NSO method [11]. After choosing
of frequency-dependent memory functions are considered,                  parameters of the reduced description, taking into account
                                                                         projections we present the nonequilibrium particle function
                                                                            (       )
and the diffusion equations with fractality of space-time are
obtained.                                                                 ρ x N ; t (as a solution of the Liouville equation) in the gene-
                                                                         ral form
   II. LIOUVILLE EQUATION WITH FRACTIONAL
DERIVATIVES FOR SYSTEM OF CLASSICAL PARTICLES                                                          ( )
                                                                                ρ ( x N ; t ) = ρ rel x N ; t
                                                                                                                                                                    (5)
                                                                                                 ∫
                                                                                                    t
   We use the Liouville equation with fractional derivatives                                    − eε (t ′−t )T (t , t ′)(1 − Prel (t ′))iLα ρ rel ( x N ; t ′)dt ′,
                                                                                                   −∞
obtained by Tarasov in Refs. [14] for a nonequilibrium partic-
le function ρ ( x N ; t ) of a classical system



                           ACIT 2018, June 1-3, 2018, Ceske Budejovice, Czech Republic
                                                                                                      76

where T (t , t ′) = exp+ − ∫ (1 − Prel (t ′))iLα dt ′ is the evolution
                             t                                                                             It is important to note that the relevant distribution function
                          t ′                                                                          corresponded to the Gibbs entropy follows from (8) at q = 1
operator in time containing the projection, exp+ is ordered                                                [5]. In the general case of the parameters 〈 Pˆ ( x)〉 t of the re-               n       α
exponential, ε → +0 after taking the thermodynamic limit,                                                  duced description of nonequilibrium processes according to
 Prel (t ′) is the generalized Kawasaki-Gunton projection ope-                                             (5) and (8), we get NSO in the form
rator depended on a structure of the relevant statistical opera-                                            ρ (t ) = ρ rel (t )
tor (distribution function), ρ rel ( x N ; t ′) . By using Zubarev’s                                                                     t
                                                                                                                                                                                                              (11)
NSO method [11], [12] and approach, ρ rel x ; t ′ will be             (    N
                                                                                   )
                                                                                                              +   ∑∫                     ∫
                                                                                                                        dµα ( x) eε (t ′−t )T (t , t ′) I n ( x; t ′) ρ rel (t ′) βFn* ( x; t ′)dt ′,
                                                                                                                   n                     −∞
found from the extremum of the Renyi entropy at fixed valu-                                                                                                         Fn ( x; t ′)
                                                                                                           where F ( x; t ′) =
                                                                                                                          *
                                                                                                                                                                                                          ,
es of observed values 〈 Pˆn ( x)〉 αt , taking into account the nor-
                                                                                                                                                             ∑∫dµ ( x) F ( x; t ′) P ( x)
                                                                                                                         n                            q −1                                          t
                                                                                                                                                 1+    q            α        n             n        α
malization condition 〈1〉 αt , rel = 1 , where the nonequilibrium                                                                                              n


average values are found respectively [5],                                                                                           I n ( x; t ′) = (1 − P(t ) ) 1q ψ −1 (t )iLα Pˆn ( x)                    (12)
             〈 Pˆn ( x)〉 αt = Iˆα (1, , N )Tˆ (1, , N ) Pˆn ρ ( x N ; t ). (6)                           are the generalized flows, P(t ) is the Mori projection opera-
 ˆI α (1, , N ) has the following form for a system of N par-                                             tor [5], and the function ψ (t ) has the following structure
                                                                            
ticles Iˆα (1, , N ) = Iˆα (1), , Iˆα ( N ), Iˆα ( j ) = Iˆα (r j ) Iˆα ( p j )                          ψ (t ) = 1 − qq−1 ∑ ∫dµα ( x) Fn ( x; t) Pn ( x).
                                                                                                                                     n
and defines operation of integration                                                                           By using the nonequilibrium statistical operator (11), we
                                      ∞                                   | x |α                           get the generalized transport equation for the parameters
          Iˆα ( x) f ( x) =       ∫
                                  −∞
                                          f ( x)dµα ( x), dµα ( x) =
                                                                          Γ(α )
                                                                                 dx.            (7)
                                                                                                           〈 Pˆn ( x)〉 αt of the reduced description,
The operator Tˆ (1, , N ) = Tˆ (1), , Tˆ ( N ) defines the opera-                                           ∂ ˆ
                                                                                                                 〈 Pn ( x)〉 αt = 〈iLα Pˆn ( x)〉 αt , rel
tion   Tˆ ( x ) f ( x ) = 1 ( f ( , x′ − x ,) + f ( , x′ + x ,)).                                         ∂t
                      j       j           2          j   j                     j         j                                                                                                                    (13)
                                                                                                                                                      t
Accordingly, the average value, which is calculated with the                                                           + ∑ ∫dµα ( x′) ∫ eε (t ′−t )ϕ P P ( x, x′; t , t ′) βFn*′ ( x′; t ′)dt ′,
                                                                                                                                                                    n n′
relevant distribution function, is defined as                                                                              n′                         −∞
        〈 ()〉 αt ,rel = Iˆα (1, , N )Tˆ (1, , N )() ρ rel ( x N ; t ).                                 where
According to Ref. [12], from the extremum of the Renyi                                                                  ϕ P P ( x, x′; t , t ′) = Iˆα (1, , N )Tˆ (1, , N )
                                                                                                                              n n′


                                                                                                                                         (                                                          )
entropy functional                                                                                                                                                                    (14)
                 1                                                                                                       × iLα Pˆn ( x)T (t , t ′) I n′ ( x′; t ′) ρ rel ( x N ; t ′)
  LR ( ρ ′) =          ln Iˆα (1, , N )Tˆ (1, , N )( ρ ′(t )) q
              1− q                                                                                         are the generalized transport kernels (the memory functions),
                                                                                                           which describe dissipative processes in the system. To de-
         − γIˆα (1, , N )Tˆ (1, , N ) ρ ′(t )                                                            monstrate the structure of the transport equations (13) and the
          −   ∑∫dµ ( x) F ( x; t ) Iˆ (1,, N )Tˆ (1,, N ) Pˆ ( x) ρ ′(t )
                  n
                          α           n
                                                α
                                                                               n
                                                                                                           transport kernels (14), we will consider, for example, diffu-
                                                                                                           sion processes. In the next section, we obtain generalized
                                                                                                           transport equations with fractional derivatives and consider a
at fixed values of observed values 〈 Pˆn ( x)〉 αt and the condition
                                                                                                           concrete example of diffusion processes of the particle in
of normalization Iˆα (1, , N )Tˆ (1, , N ) ρ ′(t ) = 1 , the relevant                                    non-homogeneous media.
distribution function takes the form
                                                                                        1
                                                                                                                III. GENERALIZED DIFFUSION EQUATIONS WITH
                    1  q −1                                                        q −1                               FRACTIONAL DERIVATIVES
   ρ rel (t ) =             1 −
                  Z R (t )     q        n
                                                    ∑∫
                                   β  H − dµα ( x) Fn ( x; t )δPˆn ( x; t ) 
                                                                               
                                                                                              , (8)
                                                                                                              One of main parameters of the reduced description to des-
                                                                                                           cribe the diffusion processes of the particles in non-homo-
where Z R (t ) is the partition function of the Renyi distribu-
                                                                                                           geneous media with fractal structure is the nonequilibrium
tion, which is determined from the normalization condition                                                                                                                    
and has the form                                                                                           density of the particle numbers, 〈 Pˆn ( x)〉 αt : n(r ; t ) = 〈 nˆ (r )〉 αt ,
                                                                                                                                    
                                                                                                           where nˆ (r ) = ∑ j =1δ (r − r j ) is the microscopic density of the
                                                                                                                            N
   Z R (t ) = Iˆα (1, , N )Tˆ (1, , N )
                                                                                       1
                                                                                                           particles. The corresponding generalized diffusion equation
         q −1                                                 q −1 (9)                                          
      × 1 −    β  H −                      ∑∫
                            dµα ( x) Fn ( x; t )δPˆn ( x; t )  .                                        for n(r ; t ) can be obtained on base of Eqs. (8), (11), (13),
           q          n                                                                                       t                                                                      
                                                                                                             ∂ nˆ (r ) α ∂ α         
                                                                                                                                           t
                                                                                                                                                                               ∂ α βν * (r ' ; t ′)
The Lagrangian multiplier γ is determined by the normaliza-
                                                                                                                 ∂t       ∂r              −∞
                                                                                                                                             ∫               ∫
                                                                                                                        =  α ⋅ dµα (r ' ) eε (t ′−t ) Dq (r , r ' ; t , t ' ) ⋅
                                                                                                                                                                                      ∂r
                                                                                                                                                                                         'α          dt ′, (15)
tion condition. The parameters Fn ( x; t ) are determined from
the self-consistency conditions                                                                            where
                                                                                                                                                                                   
                    〈 Pˆn ( x)〉 αt = 〈 Pˆn ( x)〉 αt , rel . (10)                                                                         Dq (r , r ' ; t , t ′) = 〈vˆ (r )T (t , t ′)vˆ (r ' )〉 αt ,rel       (16)




                                              ACIT 2018, June 1-3, 2018, Ceske Budejovice, Czech Republic
                                                                                   77

is the generalized coefficient diffusion of the particles within                                         ∂       t
                                                                                                                           t
                                                                                                                                                 
the Renyi statistics. Averaging in Eq. (16) is performed with
                                                                                                         ∂t            −∞
                                                                                                                           ∫
                                                                                                            nˆ (r ) α = eε (t ′−t )W (t , t ′)Ψ (r ; t ′)dt ′,    (22)
the power-law Renyi distribution,
                                                                               1        where
    ρ rel (t ) =
                   1  q −1
                          1 −
                 Z R (t ) 
                                   (                 
                                                                       )
                                                                   q −1
                                  β H − ∫dµα (r )ν * (r ; t )nˆ (r )  , (17)                     
                                                                                                            ∫
                                                                                                                      ∂α                ∂α               
                                                                                               Ψ (r ; t ′) = dµα (r ′)  α ⋅ D q (r , r ′) ⋅  'α βν * (r ' ; t ′). (23)
                                q                                                                                       ∂r                    ∂r
where                                                                                      Further we apply the Fourier transform to Eq. (22), and as
       Z (t ) = Iˆα (1, , N )Tˆ (1, , N )
          R
                                                                                        a result we get in frequency representation
                                                                                                                                               
                                                                           1                                       iωn(r ; ω ) = W (ω )Ψ (r ; ω ).                  (24)
                               ( ∫                                 )
                   q −1                                          (18)
                                                         q −1                       We can represent the frequency dependence of the memory
               × 1 −     β H − dµα (r )ν * (r ; t )nˆ (r ) 
                      q                                                               function in the following form
is the partition function of the relevant distribution function,                                                                (iω )1−ξ
                                                                                                                   W (ω ) =              , 0 < ξ ≤ 1,               (25)
 H is a Hamiltonian of the system, q is the Renyi parameter                                                                     1 + iωτ
( 0 < q < 1 ).                                                                          where the introduced relaxation time τ a characterizes the
                    
   Parameter ν (r ; t ) is the chemical potential of the particles,                     particles transport processes in the system. Then Eq. (24) can
which is determined from the self-consistency condition,                                be represented as
                                                                                                                                                      
                                  t        t                                                               (1 + iωτ )iωn(r ; ω ) = (iω )1−ξ Ψ (r ; ω ).           (26)
                             nˆ (r ) = nˆ (r )
                                       α
                                                 . α , rel
                                                                  (19)
                                                                                           Further we use the Fourier transform to fractional derivati-
β = 1/k BT ( k B is the Boltzmann constant), T is the equilib-                          ves of functions,
                             
rium value of temperature, vˆ (r ) =
                                               N   
                                               j =1 j
                                                              
                                           ∑ v δ (r − r ) is the mic-
                                                               j
                                                                                                            (                   )
                                                                                                            L 0 Dt1−ξ f (t ); iω = (iω )1−ξ L( f (t ); iω ).        (27)
                                                                                        By using it, the inverse transformation of Eq. (26) to time re-
roscopic flux density of the particles. At q = 1 , the generali-
                                                                                        presentation gives the Cattaneo-type generalized diffusion
zed diffusion equation within the Renyi statistics goes into                            equation with taking into account spatial fractality,
the generalized diffusion equation within the Gibbs statistics
                                                                                                ∂2              ∂                               ∂1−ξ       
with fractional derivatives. If q = 1 and α = 1 , we obtain the                             τ 2 n(r ; t ) + n(r ; t ) = 0 Dt1−ξ Ψ (r ; t ) = 1−ξ Ψ (r ; t ), (28)
                                                                                               ∂t               ∂t                                 ∂t
generalized diffusion equation within the Gibbs statistics. In
                                                                                        which is the new Cattaneo-type generalized equation within
the Markov approximation, the generalized coefficient of
                                                                                        the Renyi statistics with multifractal time and spatial frac-
diffusion             in    time       and       space     has   the    form
                                                                                    tality. At q = 1 from Eq. (29), we get the Cattaneo-type gene-
                    ′                ′
 Dq (r , r ' ; t , t ) ≈ Dqδ (t − t )δ (r − r ' ) . And  by excluding the pa-
                                                                                       ralized equation within the Gibbs statistics with multifractal
rameter ν * (r ' ; t ′) via the self-consistency condition, we ob-                      time and spatial fractality,
tain the diffusion equation with fractional derivatives from                                  ∂2              ∂                             ∂α            
Eq. (15)                                                                                   τ 2 n(r ; t ) + n(r ; t ) = 0 Dt1−ξ ∫dµα (r ′)  α ⋅ D(r , r ′)
                                                                                             ∂t                ∂t                                ∂r
                          ∂        t               ∂ 2α                                                                                                           (29)
                          ∂t
                                    ∑
                              nˆ (r ) α = Dq 2α ν * (r ' ; t ′).
                                                   ∂ r
                                                                         (20)                               ∂α        
                                                                                                         ⋅  'α βν (r ' ; t ),
                                           b                                                               ∂r
   The generalized diffusion equation takes into account spa-                              Eqs. (28), (29) contain significant spatial non-homogeneity
tial fractality of the system and memory effects in the genera-                                   
                                                                                      in D q (r , r ′) . If we neglect spatial non-homogeneity,
lized coefficient of diffusion Dq (r , r ' ; t , t ′) within the Renyi                                                                   
                                                                                                                   D q (r , r ′) = D qδ (r − r ′),                  (30)
statistics. Obviously, spatial fractality of system influences on
transport processes of the particles that can show up as mul-                           we get the Cattaneo-type diffusion equation with fractality of
tifractal time with characteristic relaxation times. It is known                        space-time and the constant coefficients of the diffusion
                                                          
that the nonequilibrium correlation functions Dq (r , r ' ; t , t ′)                    within the Renyi statistics,
                                                                                                 ∂2              ∂                         ∂ 2α         
can not be exactly calculated, therefore the some approxima-                                 τ 2 n(r ; t ) + n(r ; t ) = 0 Dt1−ξ D q  2α βν * (r ; t ),            (31)
tions based on physical reasons are used. In the time interval                                  ∂t               ∂t                         ∂r
 −∞ ÷ t , ion transport processes in spatially non-homogeneous                          At q = 1 , we get the Cattaneo-type diffusion equation with
system can be characterized by a set of relaxation times that                           fractality of space-time and the constant coefficients of the
are associated with the nature of interaction between the par-                          diffusion within the Gibbs statistics,
ticles and particles of media with fractal structure. To show                                      ∂2              ∂                            ∂ 2α      
the multifractal time in the generalized diffusion equation, we                                 τ 2 n(r ; t ) + n(r ; t ) = 0 Dt1−ξ ∑ D  2α ν (r ; t ), (32)
                                                                                                   ∂t               ∂t                     b      ∂r
use the following approach for the generalized coefficient of
particle diffusion                                                                      It should be noted that if we put α = 1 in Eqs. (31), (32), i.e.
                                                                                    we neglect spatial fractality, we get the Cattaneo-type diffusi-
                   Dq (r , r ′; t , t ′) = W (t , t ′) D q (r , r ′), (21)
                                                                                        on equations, which were obtained in Ref. [18],
where W (t , t ′) can be defined as the time memory function.                                        ∂2              ∂                        ∂2      
In view of this, Eq. (15) can be represented as                                                   τ 2 n(r ; t ) + n(r ; t ) = 0 Dt1−ξ D  2 ν (r ; t ).             (33)
                                                                                                    ∂t               ∂t                        ∂r




                               ACIT 2018, June 1-3, 2018, Ceske Budejovice, Czech Republic
                                                                                       78

   At τ = 0 , we get an important particular case — the gene-                                    Applications. Gordon and Breach Science Publishers,
ralized diffusion equation of particles with taking into ac-                                     1st ed., 1993.
count fractality of space-time,                                                             [3] I. Podlubny and V. T. E. Kenneth, Fractional
     ∂                              ∂α             ∂α                                       Differential Equations: An Introduction to Fractional
    ∂t                   ∫
       n(r ; t ) = 0 Dt1−ξ dµα (r ′) α ⋅ D q (r , r ′) ⋅  'α βν * (r ' ; t ), (34)
                                       ∂r                 ∂r                                     Derivatives, Fractional Differential Equations, to
and by neglecting spatial non-homogeneity of the diffusion                                       Methods of Their Solution and Some of Their
                                                                                               Applications. Academic Press, 1st ed., 1998.
coefficients D q (r , r ′) , we also get the diffusion equation
                                                                                            [4] V. V. Uchaikin, Fractional Derivatives Method.
with the constant coefficients of the diffusion with the                                         Artishock-Press, Uljanovsk, 2008.
fractional derivatives within the Renyi statistics,                                         [5] P. Kostrobij, B. Markovych, O. Viznovych, and M.
                    ∂                          ∂ 2α                                            Tokarchuk, "Generalized diffusion equation with
                       n(r ; t ) = 0 Dt1−ξ D q  2α βν * (r ; t ),              (35)
                   ∂t                          ∂r                                                fractional derivatives within Renyi statistics." Journal of
   At α = 1 , τ = 0 , we get the diffusion equation with the                                     Mathematical Physics, vol. 57, pp. 093301, 2016.
constant coefficients of the diffusion without spatial fractality                           [6] P. Kostrobij, B. Markovych, O. Viznovych, and M.
within the Renyi statistics                                                                      Tokarchuk, "Generalized electrodiffusion equation with
                  ∂                           ∂2                                               fractality of space-time." Mathematical Modeling and
                      n(r ; t ) = 0 Dt1−ξ D q  2 βν * (r ; t ),                (36)             Computing, vol. 3, n. 2, pp. 163–172, 2016.
                  ∂t                          ∂r
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                                                                                                 vol. 123, pp. 739–745, 1984.
                          ∂                 ∂2        
                             n(r ; t ) = D  2 βν (r ; t ).                     (37)        [8] R. R. Nigmatullin, "On the Theory of Relaxation for
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   Let us consider another model of the memory function                                          Solidi (b), vol. 124, pp. 389–393 1984.
                                              (iω )1−ξ                                      [9] R. R. Nigmatullin, "The realization of the generalized
                               W (ω ) =                   ,                     (38)
                                           1 + (iωτ )γ −1                                        transfer equation in a medium with fractal geometry."
 then in frequency representation we get                                                         Physica Status Solidi (b), vol. 133, pp. 425–430, 1986.
                  (               )                             
                   1 + (iωτ )γ −1 iωn(r ; ω ) = (iω )1−ξ Ψ (r ; ω ).            (39)
                                                                                            [10] R. R. Nigmatullin, "Fractional integral and its physical
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                             IV. CONCLUSION                                                 [12] B. B. Markiv, R. M. Tokarchuk, P. P. Kostrobij, and M.
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                                                                                                 2011.
[14] for a system of classical particles and Zubarev’s NSO
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