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Subdiffusion Equation with Fractional Caputo Time Derivative with Respect to Another Function in Modeling Superdiffusion

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05 December 2024

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06 December 2024

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Abstract

Superdiffusion is usually defined as a random walk process of a molecule, in which the time evolution of the mean squared displacement $\sigma^2$ of the molecule is a power function of time, $\sigma^2(t)\sim t^{\gamma}$ with $\gamma\in(1,2)$. An equation with a fractional derivative of Riesz type of order $2/\gamma$ with respect to a spatial variable (fractional superdiffusion equation) is often used to describe superdiffusion. However, this equation leads to the formula $\sigma^2(t)=\kappa t^\gamma$ with $\kappa=\infty$, which in practice makes it impossible to define the parameter $\gamma$. Moreover, due to the non-local nature of this derivative, it is generally not possible to impose boundary conditions at a thin partially permeable membrane. We show a model of superdiffusion based on the equation in which there is a fractional Caputo time derivative with respect to another function $g$; the spatial derivative is of second order. By choosing the function in an appropriate way, we obtain the $g$-superdiffusion equation whose Green's function (GF) in the long time limit approaches the GF for the fractional superdiffusion equation. The GF for the $g$-superdiffusion equation generates $\sigma^2$ with finite $\kappa$. In addition, the boundary conditions at a thin membrane can be given in a similar way as for normal diffusion or subdiffusion. As an example, the filtration process, generated by a partially permeable membrane in a superdiffusive medium, is considered.

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1. Introduction

Diffusion processes are generated by a random walk of molecules. In the standard continuous time random walk (CTRW) model [1,2,3,4,5,6,7], this process is characterized by two probability densities ψ ( Δ t ) and λ ( Δ x ) describing jumps of a single particle, Δ t is the waiting time for the particle to jump, Δ x is the length of the jump. In normal diffusion, both distributions have finite moments. In the case of anomalous diffusion at least one of these distributions has a heavy tail, which causes it to have infinite moments. In the case of subdiffusion the waiting time for the molecule to jump is anomalously long, ψ has a heavy tail. Subdiffusion can occur in media in which the movement of molecules is very hindered, such as gels or porous media. When jumps of molecules can be anomalously long, which occurs in turbulent media, we are dealing with superdiffusion. In this case, λ has a heavy tail, the second central moment of this distribution is infinite. Within the CTRW model, anomalous diffusion is described by an equation with a fractional derivative, in the subdiffusion equation it is a fractional derivative with respect to time, and in the superdiffusion equation it is a fractional derivative with respect to the spatial variable [1,2,3,6,7,8,9,10,11,12,13,14,15].
Types of diffusion processes are often defined by the temporal evolution of the mean square displacement (MSD) σ 2 of a diffusing molecule [1,16,17,18,19],
σ 2 ( t ) t 2 / γ , 2 > γ > 1 , for superdiffusion , t , for normal diffusion , t α , 0 < α < 1 , for ordinary subdiffusion .
In an unbounded homogeneous one-dimensional system, there is σ 2 ( t ) = 2 D α t α / Γ ( 1 + α ) with 0 < α < 1 for subdiffusion and σ 2 ( t ) = 2 D α = 1 t for normal diffusion, D α is a subdiffusion coefficient given in the units of m 2 / sec (or normal diffusion coefficient when α = 1 ). However, for superdiffusion described by a fractional differential equation, the relation takes the form
σ 2 ( t ) = κ t 2 / γ
with κ = . Thus, for fractional superdiffusion σ 2 ( t ) = holds which is a rather useless relation because it does not define the parameter γ .
Another disadvantage of the fractional superdiffusion model is the difficulty in assigning boundary conditions at a partially permeable membrane. The reason for this is that the fractional derivative with respect to the spatial variable has a non-local character. Then, non-local boundary conditions have been used. This causes difficulties in using the fractional superdiffusion equation to model the process in membrane systems.
We propose a model of superdiffusion that leads to Eq. (2) with κ < , and in which local boundary conditions at a membrane, such as those for subdiffusion or normal diffusion, can be applied. The model is based on the g–subdiffusion equation with fractional Caputo time derivative with respect to another function, see Refs. [20,21]. The g–subdiffusion equation can be interpreted as the ordinary subdiffusion equation with a changed time scale controlled by the function g. The change in time scale is generated by a deterministic process. We add that a change in time scale can also be generated by a stochastic process in the subordinate method [6,22,23,24,25,26]. So far, the g–subdiffusion equation has been used to describe a smooth transition from subdiffusion to ultraslow diffusion (slow subdiffusion) [20], to superdiffusion [27], to subdiffusion with a changed parameter α [28], to model the transition between different types of anomalous diffusion with irreversible reactions [29], and to describe anomalous diffusion of drugs released from densely packed gel beads immersed in water [30]. In this paper, this equation is used to describe superdiffusion in the entire time domain. We consider diffusion in a one-dimensional unbounded system, except in Sec. V, where the filtration process in a membrane system is modeled.

2. Anomalous Diffusion Equations

In this section we show the ordinary subdiffusion and fractional superdiffusion equations, along with their Green’s functions. The Green’s function (GF) P ( x , t | x 0 ) is defined as the solution to the equation with the initial condition P ( x , 0 | x 0 ) = δ ( x x 0 ) , δ is the delta–Dirac function, and - in an unbounded system - with boundary conditions P ( ± , t | x 0 ) = 0 . The GF is interpreted as the probability density of finding a molecule at point x at time t, x 0 being the initial position of the molecule at time t = 0 .

2.1. Ordinary Subdiffusion Equation

The ordinary subdiffusion equation reads
C α P α ( x , t | x 0 ) t α = D α 2 P α ( x , t | x 0 ) x 2 ,
where 0 < α < 1 ,
C d α f ( t ) d t α = 1 Γ ( 1 α ) 0 t ( t u ) α f ( u ) d u
is the fractional Caputo time derivative, f ( u ) = d f ( u ) / d u .
The Green’s function for Eq. (3) is (see, among others, Refs. [31,32,33,34,35])
P α ( x , t | x 0 ) = 1 2 D α f 1 + α / 2 , α / 2 t ; | x x 0 | D α = 1 2 D α t α j = 0 1 j ! Γ ( 1 α ( j + 1 ) / 2 ) | x x 0 | D α t α j .
Formally, the Green’s function for normal diffusion can be obtained from the Green’s function for ordinary subdiffusion Eq. (5) in the limit α 1 ; in the following this limit is also noted as α = 1 .
P α = 1 ( x , t | x 0 ) = 1 2 π D t e ( x x 0 ) 2 4 D t .
The above function fulfils the normal diffusion equation
P α = 1 ( x , t | x 0 ) t = D 2 P α = 1 ( x , t | x 0 ) x 2 .
In terms of the ordinary Laplace transform
L [ f ( t ) ] ( s ) = 0 e s t f ( t ) d t ,
due to the following relation
L C d α f ( t ) d t α ( s ) = s α L [ f ( t ) ] ( s ) s α 1 f ( 0 ) , α ( 0 , 1 ) ,
the ordinary subdiffusion equation is
s α L [ P α ( x , t | x 0 ) ] ( s ) s α 1 P α ( x , 0 | x 0 ) = D α 2 L [ P α ( x , t | x 0 ) ] ( s ) x 2 .
The solution to Eq. (10) is the Laplace transform of Green’s function,
L [ P α ( x , t | x 0 ) ] ( s ) = 1 2 D α s 1 α / 2 e | x x 0 | s α / 2 D α .

2.2. Factional Superdiffusion Equation

The fractional superdiffusion equation reads
P γ ( x , t | x 0 ) t = D γ γ P γ ( x , t | x 0 ) | x | γ ,
where the Riesz–type fractional derivative is defined by its Fourier transform, F ( k ) = e i k x f ( x ) d x , as
F d γ f ( x ) d | x | γ ( k ) = | k | γ F ( k ) .
The Green’s function for Eq. (12) is, see Ref. [27] and the references cited therein,
P γ ( x , t | x 0 ) = 1 π | x x 0 | H 12 11 | x x 0 | γ 2 γ D γ t ( 1 , 1 ) ( 1 / 2 , γ / 2 ) ( 1 , γ / 2 ) = 1 γ π ( D γ t ) 1 / γ j = 0 Γ ( 1 / γ + 2 j / γ ) j ! Γ ( 1 / 2 + j ) ( x x 0 ) 2 4 ( D γ t ) 2 / γ j ,
where H denotes the H–Fox function [36].

3. G –Subdiffusion Equation

The g–subdiffusion equation is a modified ordinary subdiffusion equation Eq. (3). The modification consists in changing the time variable t to a function g ( t ) ,
t g ( t ) ,
g ( t ) is given in a time unit and meets the conditions
g ( 0 ) = 0 , g ( ) = , g ( t ) > 0 .
In order to determine the equation and Green’s function for the g–subdiffusion process, the Laplace transform with respect to the function g, which is called the g–Laplace transform, can be used [37,38]
L g [ f ( t ) ] ( s ) = 0 e s g ( t ) f ( t ) g ( t ) d t .
The relation between the Laplace transforms is as follows
L g [ f ( t ) ] ( s ) = L [ f ( g 1 ( t ) ) ] ( s ) .
Eq. (18) provides the relation
L g [ f ( t ) ] ( s ) = L [ h ( t ) ] ( s ) f ( t ) = h ( g ( t ) ) .
Knowing the ordinary Laplace transform, the above equation is helpful in determining the inverse g–Laplace transform. The examples are
L g 1 1 s μ + 1 ( t ) = g μ ( t ) Γ ( 1 + μ ) , μ > 1 ,
L g 1 s ν e a s β ( t ) f ν , β ( g ( t ) ; a ) = 1 g 1 + ν ( t ) j = 0 1 j ! Γ ( ν β j ) a g β ( t ) j ,
a , β > 0 .
The conclusion from Eqs. (19) is that the change in the time variable can be made according to the relation
t g ( t ) L [ P α ( x , t | x 0 ) ] ( s ) L g [ P g ( x , t | x 0 ) ] ( s ) .
Applying the rule Eq. (22) to Eq. (10), we get
s α L g [ P g , α ( x , t | x 0 ) ] ( s ) s α 1 P g , α ( x , 0 | x 0 ) = D α 2 L g [ P g , α ( x , t | x 0 ) ] ( s ) x 2 ,
where P g , α ( x , 0 | x 0 ) = δ ( x x 0 ) . Due to the relation
L g C d g α f ( t ) d t α ( s ) = s α L g [ f ( t ) ] ( s ) s α 1 f ( 0 ) , α ( 0 , 1 ) ,
where
C d g α f ( t ) d t α = 1 Γ ( 1 α ) 0 t [ g ( t ) g ( u ) ] α f ( u ) d u
is the Caputo fractional derivative with respect to another function g[21,37,38], the inverse g–Laplace transform of Eq. (24) reads
C g α P g , α ( x , t | x 0 ) t α = D α 2 P g , α ( x , t | x 0 ) x 2 .
When α 1 there is
C d g f ( t ) d t = lim α 1 C d g α f ( t ) d t α = f ( t ) g ( t ) .
Combining Eqs. (11) and (22) we get the Green’s function for g-subdiffusion equation in terms of the g-Laplace transform
L g [ P g , α ( x , t | x 0 ) ] ( s ) = 1 2 D α s 1 α / 2 e | x x 0 | s α / 2 D α .
Eqs. (21) and (28) provide
P g , α ( x , t | x 0 ) = 1 2 D α f 1 + α / 2 , α / 2 g ( t ) ; | x x 0 | D α = 1 2 D α g α ( t ) j = 0 1 j ! Γ ( 1 α ( j + 1 ) / 2 ) | x x 0 | D α g α ( t ) j .
Since P is translational invariant and symmetric with respect to the point x 0 , there is
σ 2 ( t ) = 2 0 x 2 P ( x , t | 0 ) d x .
In terms of the g-Laplace transform we have L g [ σ 2 ( t ) ] ( s ) = 0 x 2 [ P g , α ( x , t | 0 ) ] ( s ) d x = 2 D α / s 1 + α . Finally, we obtain for g-subdiffusion
σ g 2 ( t ) = 2 D α Γ ( 1 + α ) g α ( t ) .

4. Using the G –Subdiffusion Equation to Describe Superdiffusion

The idea of using the g–subdiffusion equation to describe superdiffusion is based on the definition of the function g which provides Eq. (31) in the form of Eq. (2) with finite κ .

4.1. Finding the Function g

We assume that a function g provides asymptotic agreement between the Green’s function for g–subdiffusion Eq. (29) and the one for fractional superdiffusion Eq. (14) when t ,
P g , α ( x , t | x 0 ) = P γ ( x , t | x 0 ) .
Since
P g , α ( x , t | x 0 ) = 1 2 D α Γ ( 1 α / 2 ) g α ( t ) ,
P γ ( x , t | x 0 ) = 1 γ Γ ( 1 / γ ) ( D γ t ) 1 / γ ,
we get from the above equations
g ˜ ( t ) = E t 2 γ α ,
where
E = π γ D γ 1 / γ 2 D α Γ ( 1 / γ ) Γ ( 1 α / 2 ) 2 / α ,
g ˜ is the designation of the function g for superdiffusion. We note that g α ( t ) D α = π γ D γ 1 / γ t 1 / γ / [ 2 Γ ( 1 / γ ) π ] , which causes the subdiffusion coefficient D α to be eliminated from the Green’s function. Eqs. (29) and (35) provide the Green’s function describing superdiffusion
P g ˜ , α ( x , t | x 0 ) = Γ ( 1 / γ ) Γ ( 1 α / 2 ) π γ ( D γ t ) 1 / γ j = 0 1 j ! Γ ( 1 α ( j + 1 / 2 ) | x x 0 | 2 Γ ( 1 / γ ) Γ ( 1 α / 2 ) π γ ( D γ t ) 1 / γ j .
The time evolution of MSD is
σ 2 ( t ) = κ g ˜ t 2 γ ,
with
κ g ˜ = π γ D γ 1 / γ 2 Γ ( 1 / γ ) Γ ( 1 α / 2 ) 2 .

4.2. G–Superdiffusion Equation

The g–superdiffusion equation, which is defined as the g–subdiffusion equation describing superdiffusion, reads
C γ , α P ( x , t | x 0 ) t γ , α = D ˜ 2 P ( x , t | x 0 ) x 2 ,
where
C γ , α f ( t ) t γ , α = 1 Γ ( 1 α ) 0 t f ( u ) ( t 2 γ α u 2 γ α ) d u ,
D ˜ is the superdiffusion coefficient given in the units of m 2 / sec 2 / γ . This coefficient is related to other parameters as D ˜ = [ π γ D γ 1 / γ / ( 2 Γ ( 1 / γ ) Γ ( 1 α / 2 ) ) ] 2 .

4.3. Stochastic Interpretation

The ordinary subdiffusion equation can be derived from the ordinary continuous time random walk (CTRW) model. The g–subdiffusion equation can be derived from a modified CTRW model (called the g-CTRW model), which becomes the ordinary CTRW model when g ( t ) t [39]. Let Δ t i be the waiting time for the particle to i-th jump. The sequences of waiting times for the particle to jump for both processes are related to each other as follows
P n [ ( Δ t 1 , Δ t 2 , , Δ t n ) o r d i n a r y s u b d i f . ] = P n [ ( g 1 ( Δ t 1 ) , g 1 ( Δ t 2 ) , , g 1 ( Δ t n ) ) g s u b d i f . ] ,
where P n is the probability distribution of the sequence of n waiting times for a particle to jump. The average number of a particle jumps for g–subdiffusion is given by the formula [27]
n ( t ) = g α ( t ) τ Γ ( 1 + α ) ,
where τ is a parameter given in the unit of sec α . The mean jumps frequency is defined as f ( t ) = d n ( t ) / d t , for g–subdiffusion there is
f ( t ) = g ( t ) τ Γ ( α ) g 1 α ( t ) .
From Eqs. (35) and (44) we get
f ( t ) = E ˜ t 2 γ 1 .
where E ˜ = 2 E α / ( γ τ Γ ( 1 + α ) ) . Eq. (45) shows that the superdiffusion effect in the g–subdiffusion process is caused by an increasing frequency of particle jumps. This is a different superdiffusion interpretation than its interpretation within the ordinary CTRW model. In the latter model the superdiffusion effect originates from anomalously long particle jumps performed with relatively high probabilities whereas jump frequency is constant.

4.4. The Influence of Parameter α on g–Superdiffusion

Example plots of the Green’s functions P γ and P g ˜ , α are shown in Figure 1; the Green’s functions have been plotted for 20 leading terms in the series defining the function. Throughout this paper, the values of all parameters and variables are given in arbitrarily chosen units. The qualitative differences between the functions are most visible at point x = 0 . The function P γ is smooth, as is the function P g ˜ , α for α 1 , while the latter functions for α < 1 has characteristic spikes at this point.
We note that the exponent of the function Eq. (38) is the same as for fractional superdiffusion and depends on the superdiffusion parameter γ only, the function κ g ˜ is finite and depends on both parameters γ and α . In order to check the influence of the parameter α on the Green’s function, we use the relative function P R showing the relative difference of the Green’s functions P g ˜ , α and P γ ,
P R ( x , t | x 0 ) = P γ ( x , t | x 0 ) P g ˜ , α ( x , t | x 0 ) P γ ( x , t | x 0 ) .
An example of the influence of the parameter α on the Green’s function is shown in Figure 2. The figure suggests that for x not too far from the initial particle position, the functions P γ and P g ˜ , α differ from each other rather little, P γ is closer to P g ˜ , α for larger α . For large x, P γ dominates over P g ˜ , α . Next we consider the detailed case of α 1 .

4.5. G-Subdiffusion for α 1

Let us write the function P γ Eq. (14) in the following form
P γ ( x , t | x 0 ) = 1 γ π ( D γ t ) 1 / γ j = 0 A j j ! ( x x 0 ) 2 4 ( D γ t ) 2 / γ j ,
where A j = Γ ( 1 / γ + 2 j / γ ) / [ j ! Γ ( 1 / 2 + j ) ] . In the limit α 1 , P g ˜ , α has a structure similar to P γ ,
P g ˜ , α 1 ( x , t | x 0 ) = 1 γ π ( D γ t ) 1 / γ j = 0 B j j ! ( x x 0 ) 2 γ ( D γ t ) 2 / γ j ,
where B j = ( Γ ( 1 / γ ) / π ) ( 2 Γ ( 1 / γ ) / π γ ) j .
The plots of the relative function
P R ( x , t | x 0 ) = P γ ( x , t | x 0 ) P g ˜ , α 1 ( x , t | x 0 ) P γ ( x , t | x 0 ) .
are shown in Figures (Figure 3) and (Figure 4), here D γ = 10 , and x 0 = 0 . Figure 3 shows that the range of x in which both Green’s functions are close to each other grows with time. Figure 4 shows that for larger values of the parameter γ (which corresponds to a smaller superdiffusion effect) the relation P γ P g ˜ , α 1 holds in a larger range of x.
Plots of the Green’s functions P γ and P g ˜ , α for different times are shown in Figure 5, Figure 6 and Figure 7 for γ = 1.5 , D γ = 10 , and x 0 = 0 . The plots suggest that both functions are rather close to each other for both short and long times, their qualitative features are also similar.

5. Filtration in a Superdiffusion System

As mentioned, using fractional superdiffusion equations one cannot uniquely define local boundary conditions at a thin membrane, excluding boundary conditions at fully absorbing or fully reflecting walls [40]. The boundary conditions used for this equation are usually non-local, which - in our opinion - causes difficulties in their physical interpretation. However, for the g–superdiffusion equation local boundary conditions can be used because the equation contains an integer-order spatial derivative; these conditions are in practice the same as boundary conditions for ordinary subdiffusion or normal diffusion equations.
The membrane can be used to filter a diffusing substance. Assuming the system is homogeneous in the plane parallel to the membrane, the problem is one-dimensional. Let a thin membrane, placed at point x = 0 , separates vessels A and B. We assume that initially a diffusing molecule is in the vessel A, x 0 < 0 . The filtering membrane allows (almost) free movement of molecules from A to B, while molecules trying to pass through the membrane in the opposite direction can be retained at the membrane with probability σ . Let us assume that the walls bounded the vessels are located at a large distance from the membrane and do not effectively affect the diffusion of molecules through the membrane. Then, the vessels are represented as infinite intervals, A = ( , 0 ) and B = ( 0 , ) .
The boundary conditions at the membrane are [41]
J A , g ˜ , α ( 0 , t | x 0 ) = J B , g ˜ , α ( 0 + , t | x 0 ) ,
and
P A , g ˜ , α ( 0 , t | x 0 ) = σ P B , g ˜ , α ( 0 + , t | x 0 ) ,
where the g–superdiffusion flux J g ˜ , α is defined as
J g ˜ , α ( x , s | x 0 ) = D α C g ˜ α t α P g ˜ , α ( x , t | x 0 ) x .
The above boundary conditions generate the following Green’s functions (see Ref. [41])
P A , g ˜ , α ( x , t | x 0 ) = P g ˜ , α ( x , t | x 0 ) + ( 1 Λ ) P g ˜ , α ( x , t | 2 x M x 0 ) ,
P B , g ˜ , α ( x , t | x 0 ) = Λ P g ˜ , α ( x , t | x 0 ) ,
where Λ = 2 σ / ( 1 + σ ) .
As example, we consider a filtration process taking place in a subdiffusive medium, such as a turbulent one, in which at the initial moment a homogeneous solution of concentration C 0 is in region A and there is no diffusing substance in region B. The initial conditions are C A ( x , 0 ) = C 0 and C B ( x , 0 ) = 0 . We are interested in the temporal evolution of the amount of substance in region B. The concentration C B ( x , t ) can be calculated using the formula
C B , g ˜ , α ( x , t ) = C 0 0 P B , g ˜ , α ( x , t | x 0 ) d x 0 .
Eq. (55) provide
C B , g ˜ , α ( x , t ) = Λ C 0 2 f 1 , α / 2 E t 2 γ α , x D .
The time evolution of total amount of substance in region B, W B , g ˜ , α ( t ) = 0 C B , g ˜ , α ( x , t ) d x , is
W B , g ˜ , α ( t ) = Λ C 0 E α / 2 Γ ( 1 + α / 2 ) t 1 γ .
Eqs. (56) and (57) can be easily derived when we use the g–Laplace transform of the above equations and Eqs (20), (21), (28), and (35). We add that for ordinary subdiffusion with parameter α the rate of the filtration process is W B , α ( t ) t α / 2 [41]. Comparing this equation with Eq. (57) we obtain a relation showing the difference in filtration for the processes, W B , g ˜ , α ( t ) t η W B , α ( t ) with η = ( 1 / γ ) ( α / 2 ) > 0 .

6. Final Remarks

The g–subdiffusion equation with the fractional Caputo derivative with respect to another function can be interpreted as the ordinary subdiffusion equation with a changed time variable. So far, the g–subdiffusion equation has been mainly used to describe a smooth transition from subdiffusion to another type of diffusion [20,27] or subdiffusion with a changed parameter α [28]. In this paper, this equation is used to describe superdiffusion in the entire time domain. The characteristic features of the g–superdiffusion equation are as follows.
  • The g–superdiffusion equation is defined as the g–subdiffusion equation Eq. (26) with the function g given by Eq. (35). This equation can be written in the equivalent form Eq. (40), which contains a Caputo-type fractional time derivative controlled by two parameters γ ( 1 , 2 ) and α ( 0 , 1 ) . The parameter γ is the exponent of the time evolution of MSD Eq. (38), which defines the type of diffusion. This parameter also defines the order of the Riesz-type derivative with respect to the spatial variable in the fractional superdiffusion equation which gives the same Green’s function as the g–subdiffusion equation in the limit t . Thus, it can be said that these equations give an equivalent description of the process in the long-time limit. The parameter α controls the rate of convergence of the Green’s functions.
  • More general, solutions of the g–subdiffusion equation goes asymptotically to solutions of the fractional superdiffusion equation when the initial and boundary conditions, and the parameter γ are the same for both equations.
  • It appears that the parameter α for which the Green’s functions for g–superdiffusion are qualitatively most similar to the one for fractional superdiffusion is α = 1 . This case is considered in Sec. 4.E.
  • The g–subdiffusion equation is "local in space", so "typical" boundary conditions at partially permeable walls can be involved in the superdiffusion model.
  • The stochastic interpretation of g–superdiffusion process is that the jump frequency of a diffusing particle increases over time to infinity. The probability distribution of the jump lengths of a diffusing molecule has finite moments.
  • The Green’s function for g–subdiffusion provides σ 2 ( t ) = κ t 2 / γ with κ < .
An effective method for solving the g–superdiffusion equations is the method of Laplace transform with respect to the function g ˜ Eq. (35).

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Figure 1. Green’s functions for fractional subdiffusion P γ Eq. (14) (thick solid lines without symbols) and for g-superdiffusion P g ˜ , α Eq. (37) (lines with symbols) for α given in the legend, here t = 100 , D γ = 10 , and x 0 = 0 .
Figure 1. Green’s functions for fractional subdiffusion P γ Eq. (14) (thick solid lines without symbols) and for g-superdiffusion P g ˜ , α Eq. (37) (lines with symbols) for α given in the legend, here t = 100 , D γ = 10 , and x 0 = 0 .
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Figure 2. Plots of relative function P R for α given in the legend, γ = 1.5 , t = 100 , and D γ = 10 .
Figure 2. Plots of relative function P R for α given in the legend, γ = 1.5 , t = 100 , and D γ = 10 .
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Figure 3. Plots of P R Eq. (49) for times given in the legend, γ = 1.5 .
Figure 3. Plots of P R Eq. (49) for times given in the legend, γ = 1.5 .
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Figure 4. Plots of P R Eq. (49) for γ given in the legend, t = 100 .
Figure 4. Plots of P R Eq. (49) for γ given in the legend, t = 100 .
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Figure 5. Green’s functions for fractional subdiffusion P γ Eq. (14) (solid lines with filled symbols) and for g-superdiffusion P g ˜ , α Eq. (37) (dashed lines with open symbols) for times given in the legend.
Figure 5. Green’s functions for fractional subdiffusion P γ Eq. (14) (solid lines with filled symbols) and for g-superdiffusion P g ˜ , α Eq. (37) (dashed lines with open symbols) for times given in the legend.
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Figure 6. The plot description is the same as for Figure 5.
Figure 6. The plot description is the same as for Figure 5.
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Figure 7. The plot description is the same as for Figure 5.
Figure 7. The plot description is the same as for Figure 5.
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